Advanced search options

Advanced Search Options 🞨

Browse by author name (“Author name starts with…”).

Find ETDs with:

in
/  
in
/  
in
/  
in

Written in Published in Earliest date Latest date

Sorted by

Results per page:

Sorted by: relevance · author · university · dateNew search

You searched for subject:(Main sequence stars). Showing records 1 – 30 of 42 total matches.

[1] [2]

Search Limiters

Last 2 Years | English Only

▼ Search Limiters


Vanderbilt University

1. Le Blanc, Thompson S. The Role of Disks in the Angular Momentum Evolution of Young, Low-Mass Stars.

Degree: PhD, Physics, 2012, Vanderbilt University

 Detailed studies of the spectral energy distributions (SEDs) of young stars can reveal much about their basic properties and their circumstellar material. Previous work suggests… (more)

Subjects/Keywords: circumstellar material; pre-main sequence; stars; rotation

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Le Blanc, T. S. (2012). The Role of Disks in the Angular Momentum Evolution of Young, Low-Mass Stars. (Doctoral Dissertation). Vanderbilt University. Retrieved from http://hdl.handle.net/1803/13325

Chicago Manual of Style (16th Edition):

Le Blanc, Thompson S. “The Role of Disks in the Angular Momentum Evolution of Young, Low-Mass Stars.” 2012. Doctoral Dissertation, Vanderbilt University. Accessed March 05, 2021. http://hdl.handle.net/1803/13325.

MLA Handbook (7th Edition):

Le Blanc, Thompson S. “The Role of Disks in the Angular Momentum Evolution of Young, Low-Mass Stars.” 2012. Web. 05 Mar 2021.

Vancouver:

Le Blanc TS. The Role of Disks in the Angular Momentum Evolution of Young, Low-Mass Stars. [Internet] [Doctoral dissertation]. Vanderbilt University; 2012. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/1803/13325.

Council of Science Editors:

Le Blanc TS. The Role of Disks in the Angular Momentum Evolution of Young, Low-Mass Stars. [Doctoral Dissertation]. Vanderbilt University; 2012. Available from: http://hdl.handle.net/1803/13325


Rice University

2. Cauley, Paul Wilson. Diagnosing Mass Flows Around Herbig Ae/Be Stars.

Degree: PhD, Natural Sciences, 2014, Rice University

 Most stars form surrounded by a massive disk of dust and gas. As the star evolves, its interaction with the surrounding disk material has a… (more)

Subjects/Keywords: Pre-main sequence stars; Herbig Ae/Be stars/ Classical T Tauri stars; accretion; stellar winds

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Cauley, P. W. (2014). Diagnosing Mass Flows Around Herbig Ae/Be Stars. (Doctoral Dissertation). Rice University. Retrieved from http://hdl.handle.net/1911/87727

Chicago Manual of Style (16th Edition):

Cauley, Paul Wilson. “Diagnosing Mass Flows Around Herbig Ae/Be Stars.” 2014. Doctoral Dissertation, Rice University. Accessed March 05, 2021. http://hdl.handle.net/1911/87727.

MLA Handbook (7th Edition):

Cauley, Paul Wilson. “Diagnosing Mass Flows Around Herbig Ae/Be Stars.” 2014. Web. 05 Mar 2021.

Vancouver:

Cauley PW. Diagnosing Mass Flows Around Herbig Ae/Be Stars. [Internet] [Doctoral dissertation]. Rice University; 2014. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/1911/87727.

Council of Science Editors:

Cauley PW. Diagnosing Mass Flows Around Herbig Ae/Be Stars. [Doctoral Dissertation]. Rice University; 2014. Available from: http://hdl.handle.net/1911/87727


University of Western Ontario

3. Patel, Parshati. The Inner Gaseous Disks Of Herbig Be Stars.

Degree: 2016, University of Western Ontario

 Herbig Ae/Be stars are intermediate mass (~2 to 20Msun) pre-main sequence stars that inherit a circumstellar disk of dust and gas from their formation phase.… (more)

Subjects/Keywords: Herbig Ae/Be stars; Circumstellar Disks; Pre-main sequence stars; Emission Line stars; Physical Processes; Stars, Interstellar Medium and the Galaxy

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Patel, P. (2016). The Inner Gaseous Disks Of Herbig Be Stars. (Thesis). University of Western Ontario. Retrieved from https://ir.lib.uwo.ca/etd/3692

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Patel, Parshati. “The Inner Gaseous Disks Of Herbig Be Stars.” 2016. Thesis, University of Western Ontario. Accessed March 05, 2021. https://ir.lib.uwo.ca/etd/3692.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Patel, Parshati. “The Inner Gaseous Disks Of Herbig Be Stars.” 2016. Web. 05 Mar 2021.

Vancouver:

Patel P. The Inner Gaseous Disks Of Herbig Be Stars. [Internet] [Thesis]. University of Western Ontario; 2016. [cited 2021 Mar 05]. Available from: https://ir.lib.uwo.ca/etd/3692.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Patel P. The Inner Gaseous Disks Of Herbig Be Stars. [Thesis]. University of Western Ontario; 2016. Available from: https://ir.lib.uwo.ca/etd/3692

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

4. Elliott, Paul Michael. Is multiplicity universal? : a study of multiplicity in the young moving groups.

Degree: PhD, 2016, University of Exeter

 The young moving groups are collections of nearby (<200 pc), young (5-150 Myr) pre-main sequence stars; these stars offer us one of the best opportunities… (more)

Subjects/Keywords: 523.8; binaries; star formation; pre-main-sequence stars; multiplicity

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Elliott, P. M. (2016). Is multiplicity universal? : a study of multiplicity in the young moving groups. (Doctoral Dissertation). University of Exeter. Retrieved from http://hdl.handle.net/10871/21876

Chicago Manual of Style (16th Edition):

Elliott, Paul Michael. “Is multiplicity universal? : a study of multiplicity in the young moving groups.” 2016. Doctoral Dissertation, University of Exeter. Accessed March 05, 2021. http://hdl.handle.net/10871/21876.

MLA Handbook (7th Edition):

Elliott, Paul Michael. “Is multiplicity universal? : a study of multiplicity in the young moving groups.” 2016. Web. 05 Mar 2021.

Vancouver:

Elliott PM. Is multiplicity universal? : a study of multiplicity in the young moving groups. [Internet] [Doctoral dissertation]. University of Exeter; 2016. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/10871/21876.

Council of Science Editors:

Elliott PM. Is multiplicity universal? : a study of multiplicity in the young moving groups. [Doctoral Dissertation]. University of Exeter; 2016. Available from: http://hdl.handle.net/10871/21876


University of Exeter

5. Sergison, Darryl James. Untangling the signals : investigating accretion and photometric variability in young stars.

Degree: PhD, 2015, University of Exeter

 In this thesis, an assessment is made of the value of optical CMDs as a useful diagnostic of the accretion properties of young stars. An… (more)

Subjects/Keywords: 500; pre-main-sequence stars; YSOs; optical variability; accretion; discs

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Sergison, D. J. (2015). Untangling the signals : investigating accretion and photometric variability in young stars. (Doctoral Dissertation). University of Exeter. Retrieved from http://hdl.handle.net/10871/18720

Chicago Manual of Style (16th Edition):

Sergison, Darryl James. “Untangling the signals : investigating accretion and photometric variability in young stars.” 2015. Doctoral Dissertation, University of Exeter. Accessed March 05, 2021. http://hdl.handle.net/10871/18720.

MLA Handbook (7th Edition):

Sergison, Darryl James. “Untangling the signals : investigating accretion and photometric variability in young stars.” 2015. Web. 05 Mar 2021.

Vancouver:

Sergison DJ. Untangling the signals : investigating accretion and photometric variability in young stars. [Internet] [Doctoral dissertation]. University of Exeter; 2015. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/10871/18720.

Council of Science Editors:

Sergison DJ. Untangling the signals : investigating accretion and photometric variability in young stars. [Doctoral Dissertation]. University of Exeter; 2015. Available from: http://hdl.handle.net/10871/18720


University of Toledo

6. Allen, Thomas S. A Multi-wavelength survey of the Young Stellar Cluster Cep OB3b.

Degree: PhD, Physics, 2014, University of Toledo

 We present results from an extensive multi-wavelength survey of Cep OB3b, one of the largest young clusters within 1 kpc of the Sun. We estimate… (more)

Subjects/Keywords: Astronomy; pre-main sequence stars; interstellar extinction; stellar clusters

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Allen, T. S. (2014). A Multi-wavelength survey of the Young Stellar Cluster Cep OB3b. (Doctoral Dissertation). University of Toledo. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=toledo1404697742

Chicago Manual of Style (16th Edition):

Allen, Thomas S. “A Multi-wavelength survey of the Young Stellar Cluster Cep OB3b.” 2014. Doctoral Dissertation, University of Toledo. Accessed March 05, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=toledo1404697742.

MLA Handbook (7th Edition):

Allen, Thomas S. “A Multi-wavelength survey of the Young Stellar Cluster Cep OB3b.” 2014. Web. 05 Mar 2021.

Vancouver:

Allen TS. A Multi-wavelength survey of the Young Stellar Cluster Cep OB3b. [Internet] [Doctoral dissertation]. University of Toledo; 2014. [cited 2021 Mar 05]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=toledo1404697742.

Council of Science Editors:

Allen TS. A Multi-wavelength survey of the Young Stellar Cluster Cep OB3b. [Doctoral Dissertation]. University of Toledo; 2014. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=toledo1404697742

7. Contreras Peña, Carlos Eduardo. Exteme variables in star forming regions.

Degree: PhD, 2015, University of Hertfordshire

 The notion that low- to intermediate-mass young stellar objects (YSOs) gain mass at a constant rate during the early stages of their evolution appears to… (more)

Subjects/Keywords: 523.8; stars: AGB and post-AGB; stars: low-mass; stars: pre-main-sequence; stars: protostars; stars: variables: T Tauri, Herbig Ae/Be; infrared: stars

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Contreras Peña, C. E. (2015). Exteme variables in star forming regions. (Doctoral Dissertation). University of Hertfordshire. Retrieved from http://hdl.handle.net/2299/15590

Chicago Manual of Style (16th Edition):

Contreras Peña, Carlos Eduardo. “Exteme variables in star forming regions.” 2015. Doctoral Dissertation, University of Hertfordshire. Accessed March 05, 2021. http://hdl.handle.net/2299/15590.

MLA Handbook (7th Edition):

Contreras Peña, Carlos Eduardo. “Exteme variables in star forming regions.” 2015. Web. 05 Mar 2021.

Vancouver:

Contreras Peña CE. Exteme variables in star forming regions. [Internet] [Doctoral dissertation]. University of Hertfordshire; 2015. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/2299/15590.

Council of Science Editors:

Contreras Peña CE. Exteme variables in star forming regions. [Doctoral Dissertation]. University of Hertfordshire; 2015. Available from: http://hdl.handle.net/2299/15590


University of Rochester

8. Pecaut, Mark (1975 - ). The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association.

Degree: PhD, 2013, University of Rochester

 We present a study of the star-formation history and accretion disk fraction of ∼0.6- 1.8 M⊙ stars in the nearest OB Association, Scorpius-Centaurus (Sco-Cen; 10-20… (more)

Subjects/Keywords: Accretion disk fraction; Intrinsic colors; Pre-main sequence stars; Scorpius-Centaurus; Stellar ages; Stellar temperatures

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Pecaut, M. (. -. ). (2013). The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association. (Doctoral Dissertation). University of Rochester. Retrieved from http://hdl.handle.net/1802/27871

Chicago Manual of Style (16th Edition):

Pecaut, Mark (1975 - ). “The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association.” 2013. Doctoral Dissertation, University of Rochester. Accessed March 05, 2021. http://hdl.handle.net/1802/27871.

MLA Handbook (7th Edition):

Pecaut, Mark (1975 - ). “The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association.” 2013. Web. 05 Mar 2021.

Vancouver:

Pecaut M(-). The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association. [Internet] [Doctoral dissertation]. University of Rochester; 2013. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/1802/27871.

Council of Science Editors:

Pecaut M(-). The star-formation history and accretion disk fraction of the Scorpius-Centaurus OB Association. [Doctoral Dissertation]. University of Rochester; 2013. Available from: http://hdl.handle.net/1802/27871

9. Vieira, Rodrigo Georgetti. Envoltórios circunstelares de estrelas jovens de massa intermediária .

Degree: PhD, Astronomia, 2012, University of São Paulo

As estrelas Herbig Ae/Be (HAeBe) representam os objetos de massa intermediária (2-10 Msol) na pré-sequência principal. Algumas de suas propriedades físicas são pouco compreendidas até… (more)

Subjects/Keywords: circumstellar material; estrelas; material circunstelar; pre-main sequence; pré-sequência principal; stars

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Vieira, R. G. (2012). Envoltórios circunstelares de estrelas jovens de massa intermediária . (Doctoral Dissertation). University of São Paulo. Retrieved from http://www.teses.usp.br/teses/disponiveis/14/14131/tde-08112012-160406/ ;

Chicago Manual of Style (16th Edition):

Vieira, Rodrigo Georgetti. “Envoltórios circunstelares de estrelas jovens de massa intermediária .” 2012. Doctoral Dissertation, University of São Paulo. Accessed March 05, 2021. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-08112012-160406/ ;.

MLA Handbook (7th Edition):

Vieira, Rodrigo Georgetti. “Envoltórios circunstelares de estrelas jovens de massa intermediária .” 2012. Web. 05 Mar 2021.

Vancouver:

Vieira RG. Envoltórios circunstelares de estrelas jovens de massa intermediária . [Internet] [Doctoral dissertation]. University of São Paulo; 2012. [cited 2021 Mar 05]. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-08112012-160406/ ;.

Council of Science Editors:

Vieira RG. Envoltórios circunstelares de estrelas jovens de massa intermediária . [Doctoral Dissertation]. University of São Paulo; 2012. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-08112012-160406/ ;

10. Pelisoli, Ingrid Domingos. White dwarf and subdwarf stars in the sloan digital sky survey.

Degree: 2018, Universidade do Rio Grande do Sul

White dwarf stars are the final observable evolutionary state of over 95% of stars and also a common outcome in binary evolution. Therefore, studying white… (more)

Subjects/Keywords: Anãs brancas; Stars; Stellar evolution; Estrelas; Evolucao estelar; White dwarfs; Estrelas binarias; Subdwarfs; Main sequence

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Pelisoli, I. D. (2018). White dwarf and subdwarf stars in the sloan digital sky survey. (Thesis). Universidade do Rio Grande do Sul. Retrieved from http://hdl.handle.net/10183/180510

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Pelisoli, Ingrid Domingos. “White dwarf and subdwarf stars in the sloan digital sky survey.” 2018. Thesis, Universidade do Rio Grande do Sul. Accessed March 05, 2021. http://hdl.handle.net/10183/180510.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Pelisoli, Ingrid Domingos. “White dwarf and subdwarf stars in the sloan digital sky survey.” 2018. Web. 05 Mar 2021.

Vancouver:

Pelisoli ID. White dwarf and subdwarf stars in the sloan digital sky survey. [Internet] [Thesis]. Universidade do Rio Grande do Sul; 2018. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/10183/180510.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Pelisoli ID. White dwarf and subdwarf stars in the sloan digital sky survey. [Thesis]. Universidade do Rio Grande do Sul; 2018. Available from: http://hdl.handle.net/10183/180510

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

11. Koutoulaki, Maria-Kalliopi. A closer look at protoplanetary discs : the inner few au probed with spectroscopy and optical interferometry.

Degree: 2020, University College Dublin. School of Physics

A first step towards understanding planetary formation is the characterisation of the structure and evolution of protoplanetary discs. Although the large scale disc is understood… (more)

Subjects/Keywords: Protoplanetary discs; Bracket gamma line; CO overtone emission; Pre-main sequence stars

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Koutoulaki, M. (2020). A closer look at protoplanetary discs : the inner few au probed with spectroscopy and optical interferometry. (Thesis). University College Dublin. School of Physics. Retrieved from http://hdl.handle.net/10197/11663

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Koutoulaki, Maria-Kalliopi. “A closer look at protoplanetary discs : the inner few au probed with spectroscopy and optical interferometry.” 2020. Thesis, University College Dublin. School of Physics. Accessed March 05, 2021. http://hdl.handle.net/10197/11663.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Koutoulaki, Maria-Kalliopi. “A closer look at protoplanetary discs : the inner few au probed with spectroscopy and optical interferometry.” 2020. Web. 05 Mar 2021.

Vancouver:

Koutoulaki M. A closer look at protoplanetary discs : the inner few au probed with spectroscopy and optical interferometry. [Internet] [Thesis]. University College Dublin. School of Physics; 2020. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/10197/11663.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Koutoulaki M. A closer look at protoplanetary discs : the inner few au probed with spectroscopy and optical interferometry. [Thesis]. University College Dublin. School of Physics; 2020. Available from: http://hdl.handle.net/10197/11663

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

12. Giarrusso, Marina. Lithium and age of pre-main sequence stars.

Degree: 2016, Università degli Studi di Catania

 The expectation to date the age of low mass pre-main sequence stars from lithium has been tested by comparing the observed lithium and the predicted… (more)

Subjects/Keywords: Area 02 - Scienze fisiche; Astrophysics, nuclear, stars, pre-main sequence, binary, lithium

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Giarrusso, M. (2016). Lithium and age of pre-main sequence stars. (Thesis). Università degli Studi di Catania. Retrieved from http://hdl.handle.net/10761/3892

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Giarrusso, Marina. “Lithium and age of pre-main sequence stars.” 2016. Thesis, Università degli Studi di Catania. Accessed March 05, 2021. http://hdl.handle.net/10761/3892.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Giarrusso, Marina. “Lithium and age of pre-main sequence stars.” 2016. Web. 05 Mar 2021.

Vancouver:

Giarrusso M. Lithium and age of pre-main sequence stars. [Internet] [Thesis]. Università degli Studi di Catania; 2016. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/10761/3892.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Giarrusso M. Lithium and age of pre-main sequence stars. [Thesis]. Università degli Studi di Catania; 2016. Available from: http://hdl.handle.net/10761/3892

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

13. Canty, James Ignatius. Investigating the properties of brown dwarfs using intermediate-resolution spectroscopy.

Degree: PhD, 2015, University of Hertfordshire

 This thesis is an investigation into some properties of brown dwarfs using medium-resolution spectroscopy. In the first part of the thesis, I address the issue… (more)

Subjects/Keywords: 523.8; stars: formation; pre-main sequence; low-mass; brown dwarfs; atmospheres; luminosity function; mass function

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Canty, J. I. (2015). Investigating the properties of brown dwarfs using intermediate-resolution spectroscopy. (Doctoral Dissertation). University of Hertfordshire. Retrieved from http://hdl.handle.net/2299/15194

Chicago Manual of Style (16th Edition):

Canty, James Ignatius. “Investigating the properties of brown dwarfs using intermediate-resolution spectroscopy.” 2015. Doctoral Dissertation, University of Hertfordshire. Accessed March 05, 2021. http://hdl.handle.net/2299/15194.

MLA Handbook (7th Edition):

Canty, James Ignatius. “Investigating the properties of brown dwarfs using intermediate-resolution spectroscopy.” 2015. Web. 05 Mar 2021.

Vancouver:

Canty JI. Investigating the properties of brown dwarfs using intermediate-resolution spectroscopy. [Internet] [Doctoral dissertation]. University of Hertfordshire; 2015. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/2299/15194.

Council of Science Editors:

Canty JI. Investigating the properties of brown dwarfs using intermediate-resolution spectroscopy. [Doctoral Dissertation]. University of Hertfordshire; 2015. Available from: http://hdl.handle.net/2299/15194


McMaster University

14. Klassen, Mikhail. Simulating Protostellar Evolution and Radiative Feedback in the Cluster Environment.

Degree: MSc, 2011, McMaster University

Stars form in clusters amidst complex and coupled physical phenomena. Among the most important of these is radiative feedback, which heats the surrounding gas… (more)

Subjects/Keywords: star formation; molecular clouds; HII regions; protostellar evolution; pre-main-sequence stars; numerical simulation; Stars, Interstellar Medium and the Galaxy; Stars, Interstellar Medium and the Galaxy

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Klassen, M. (2011). Simulating Protostellar Evolution and Radiative Feedback in the Cluster Environment. (Masters Thesis). McMaster University. Retrieved from http://hdl.handle.net/11375/11313

Chicago Manual of Style (16th Edition):

Klassen, Mikhail. “Simulating Protostellar Evolution and Radiative Feedback in the Cluster Environment.” 2011. Masters Thesis, McMaster University. Accessed March 05, 2021. http://hdl.handle.net/11375/11313.

MLA Handbook (7th Edition):

Klassen, Mikhail. “Simulating Protostellar Evolution and Radiative Feedback in the Cluster Environment.” 2011. Web. 05 Mar 2021.

Vancouver:

Klassen M. Simulating Protostellar Evolution and Radiative Feedback in the Cluster Environment. [Internet] [Masters thesis]. McMaster University; 2011. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/11375/11313.

Council of Science Editors:

Klassen M. Simulating Protostellar Evolution and Radiative Feedback in the Cluster Environment. [Masters Thesis]. McMaster University; 2011. Available from: http://hdl.handle.net/11375/11313


University of Exeter

15. Bell, Cameron Pearce MacDonald. A critical assessment of ages derived using pre-main-sequence isochrones in colour-magnitude diagrams.

Degree: PhD, 2012, University of Exeter

 In this thesis a critical assessment of the ages derived using theoretical pre-main-sequence (pre-MS) stellar evolutionary models is presented by comparing the predictions to the… (more)

Subjects/Keywords: 523.88; stars: evolution; stars: formation; stars: pre-main-sequence; techniques: photometric; open clusters and associations: general; Hertzsprung-Russell and colour-magnitude diagrams

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Bell, C. P. M. (2012). A critical assessment of ages derived using pre-main-sequence isochrones in colour-magnitude diagrams. (Doctoral Dissertation). University of Exeter. Retrieved from https://ore.exeter.ac.uk/repository/handle/10036/4017 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.571885

Chicago Manual of Style (16th Edition):

Bell, Cameron Pearce MacDonald. “A critical assessment of ages derived using pre-main-sequence isochrones in colour-magnitude diagrams.” 2012. Doctoral Dissertation, University of Exeter. Accessed March 05, 2021. https://ore.exeter.ac.uk/repository/handle/10036/4017 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.571885.

MLA Handbook (7th Edition):

Bell, Cameron Pearce MacDonald. “A critical assessment of ages derived using pre-main-sequence isochrones in colour-magnitude diagrams.” 2012. Web. 05 Mar 2021.

Vancouver:

Bell CPM. A critical assessment of ages derived using pre-main-sequence isochrones in colour-magnitude diagrams. [Internet] [Doctoral dissertation]. University of Exeter; 2012. [cited 2021 Mar 05]. Available from: https://ore.exeter.ac.uk/repository/handle/10036/4017 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.571885.

Council of Science Editors:

Bell CPM. A critical assessment of ages derived using pre-main-sequence isochrones in colour-magnitude diagrams. [Doctoral Dissertation]. University of Exeter; 2012. Available from: https://ore.exeter.ac.uk/repository/handle/10036/4017 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.571885


North-West University

16. Czanik, Robert Johann. An optical study of the high mass star forming region RCW 34 / Robert Johann Czanik .

Degree: 2013, North-West University

 This study consisted of an optical photometric and spectroscopic analysis on a 7′ 7′ field around the Southern high mass star forming region RCW 34.… (more)

Subjects/Keywords: RCW 34; T Tauri; GUM 19; HII region; Pre-main sequence stars; Star formation; Photometry; Spectroscopy; SAAO; IRAF; DANDICAM

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Czanik, R. J. (2013). An optical study of the high mass star forming region RCW 34 / Robert Johann Czanik . (Thesis). North-West University. Retrieved from http://hdl.handle.net/10394/9102

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Czanik, Robert Johann. “An optical study of the high mass star forming region RCW 34 / Robert Johann Czanik .” 2013. Thesis, North-West University. Accessed March 05, 2021. http://hdl.handle.net/10394/9102.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Czanik, Robert Johann. “An optical study of the high mass star forming region RCW 34 / Robert Johann Czanik .” 2013. Web. 05 Mar 2021.

Vancouver:

Czanik RJ. An optical study of the high mass star forming region RCW 34 / Robert Johann Czanik . [Internet] [Thesis]. North-West University; 2013. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/10394/9102.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Czanik RJ. An optical study of the high mass star forming region RCW 34 / Robert Johann Czanik . [Thesis]. North-West University; 2013. Available from: http://hdl.handle.net/10394/9102

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

17. Blevins, Sandra Melissa. The Distribution of Volatiles in Protoplanetary Disks.

Degree: 2016, The Catholic University of America

Degree Awarded: Ph.D. Physics. The Catholic University of America

This dissertation addresses several distinct goals, all relating to the distribution of molecular gas in planet-forming… (more)

Subjects/Keywords: Astrophysics; Chemistry; Astronomy; astrochemistry; infrared spectroscopy; molecular spectroscopy; planet formation; pre-main sequence stars; protoplanetary disks

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Blevins, S. M. (2016). The Distribution of Volatiles in Protoplanetary Disks. (Thesis). The Catholic University of America. Retrieved from http://hdl.handle.net/1961/cuislandora:30403

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Blevins, Sandra Melissa. “The Distribution of Volatiles in Protoplanetary Disks.” 2016. Thesis, The Catholic University of America. Accessed March 05, 2021. http://hdl.handle.net/1961/cuislandora:30403.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Blevins, Sandra Melissa. “The Distribution of Volatiles in Protoplanetary Disks.” 2016. Web. 05 Mar 2021.

Vancouver:

Blevins SM. The Distribution of Volatiles in Protoplanetary Disks. [Internet] [Thesis]. The Catholic University of America; 2016. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/1961/cuislandora:30403.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Blevins SM. The Distribution of Volatiles in Protoplanetary Disks. [Thesis]. The Catholic University of America; 2016. Available from: http://hdl.handle.net/1961/cuislandora:30403

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

18. Horenstein, Daniel. A New All-sky Catalogue of Candidate Protoplanetary Disks from Aggregated Optical and Infrared Surveys.

Degree: MS, Physics and Astronomy, 2017, Georgia State University

  To guide research into formation scenarios for giant planets, I present a catalogue of 199,391 sources with candidate protoplanetary disks. These candidates are identified… (more)

Subjects/Keywords: protoplanetary disks; stars: pre-main sequence; surveys

…capture both main sequence stars that emit primarily at optical wavelengths and stars with… …gaseous envelopes from the pre-main sequence circumstellar material (Pollack et al. 1996… …collapsed into a disk but before the protostar has reached the zero-age main sequence. While the… …main sequence in a few color-color plots for these intermediate fields, reddening was… …v CHAPTER 0 LIST OF TABLES Table 2.1 Literature Sources of Stars with Known… 

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Horenstein, D. (2017). A New All-sky Catalogue of Candidate Protoplanetary Disks from Aggregated Optical and Infrared Surveys. (Thesis). Georgia State University. Retrieved from https://scholarworks.gsu.edu/phy_astr_theses/21

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Horenstein, Daniel. “A New All-sky Catalogue of Candidate Protoplanetary Disks from Aggregated Optical and Infrared Surveys.” 2017. Thesis, Georgia State University. Accessed March 05, 2021. https://scholarworks.gsu.edu/phy_astr_theses/21.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Horenstein, Daniel. “A New All-sky Catalogue of Candidate Protoplanetary Disks from Aggregated Optical and Infrared Surveys.” 2017. Web. 05 Mar 2021.

Vancouver:

Horenstein D. A New All-sky Catalogue of Candidate Protoplanetary Disks from Aggregated Optical and Infrared Surveys. [Internet] [Thesis]. Georgia State University; 2017. [cited 2021 Mar 05]. Available from: https://scholarworks.gsu.edu/phy_astr_theses/21.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Horenstein D. A New All-sky Catalogue of Candidate Protoplanetary Disks from Aggregated Optical and Infrared Surveys. [Thesis]. Georgia State University; 2017. Available from: https://scholarworks.gsu.edu/phy_astr_theses/21

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

19. Khorrami, Zeinab. Imagerie à haute résolution des amas R136 et NGC3603 dévoilent la nature de leurs populations stellaires : A sharpened close-up of R136 and NGC3603 : unshrouding the nature of their stellar population.

Degree: Docteur es, Astrophysique relativiste, 2016, Nice

Cette thèse a pour objectif de comprendre les différents aspects de l'évolution des amas d’étoiles massives NGC3603 et R136 qui possèdent les étoiles les plus… (more)

Subjects/Keywords: Amas stellaires : individuel (R136, NGC3603); Étoiles : étoiles massives; Étoiles : imagerie; Étoiles : fonction de masse luminosité; Étoiles : pré-séquence principale; Étoiles : séquence principale; Instrumentation : haute résolution angulaire; Méthodes : numérique; Méthodes : observationnelle; Star clusters: individual (R136, NGC3603); Stars: imaging; Stars: luminosity function, mass function; Stars: massive; Stars: pre-main sequence; Stars: main sequence; Instrumentation: high angular resolution; Methods: numerical; Methods: observational

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Khorrami, Z. (2016). Imagerie à haute résolution des amas R136 et NGC3603 dévoilent la nature de leurs populations stellaires : A sharpened close-up of R136 and NGC3603 : unshrouding the nature of their stellar population. (Doctoral Dissertation). Nice. Retrieved from http://www.theses.fr/2016NICE4030

Chicago Manual of Style (16th Edition):

Khorrami, Zeinab. “Imagerie à haute résolution des amas R136 et NGC3603 dévoilent la nature de leurs populations stellaires : A sharpened close-up of R136 and NGC3603 : unshrouding the nature of their stellar population.” 2016. Doctoral Dissertation, Nice. Accessed March 05, 2021. http://www.theses.fr/2016NICE4030.

MLA Handbook (7th Edition):

Khorrami, Zeinab. “Imagerie à haute résolution des amas R136 et NGC3603 dévoilent la nature de leurs populations stellaires : A sharpened close-up of R136 and NGC3603 : unshrouding the nature of their stellar population.” 2016. Web. 05 Mar 2021.

Vancouver:

Khorrami Z. Imagerie à haute résolution des amas R136 et NGC3603 dévoilent la nature de leurs populations stellaires : A sharpened close-up of R136 and NGC3603 : unshrouding the nature of their stellar population. [Internet] [Doctoral dissertation]. Nice; 2016. [cited 2021 Mar 05]. Available from: http://www.theses.fr/2016NICE4030.

Council of Science Editors:

Khorrami Z. Imagerie à haute résolution des amas R136 et NGC3603 dévoilent la nature de leurs populations stellaires : A sharpened close-up of R136 and NGC3603 : unshrouding the nature of their stellar population. [Doctoral Dissertation]. Nice; 2016. Available from: http://www.theses.fr/2016NICE4030


University of Michigan

20. Espaillat, Catherine C. The Evolution of Dusty Disks Around Low-Mass Pre-Main Sequence Stars.

Degree: PhD, Astronomy and Astrophysics, 2009, University of Michigan

 The evolution of protoplanetary disks is intricately tied to the origin of planets. The details of how these disks evolve from initially well-mixed distributions of… (more)

Subjects/Keywords: Low-mass Pre-main Sequence Stars; Accretion Disks; T Tauri Stars; Astronomy; Science

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Espaillat, C. C. (2009). The Evolution of Dusty Disks Around Low-Mass Pre-Main Sequence Stars. (Doctoral Dissertation). University of Michigan. Retrieved from http://hdl.handle.net/2027.42/63766

Chicago Manual of Style (16th Edition):

Espaillat, Catherine C. “The Evolution of Dusty Disks Around Low-Mass Pre-Main Sequence Stars.” 2009. Doctoral Dissertation, University of Michigan. Accessed March 05, 2021. http://hdl.handle.net/2027.42/63766.

MLA Handbook (7th Edition):

Espaillat, Catherine C. “The Evolution of Dusty Disks Around Low-Mass Pre-Main Sequence Stars.” 2009. Web. 05 Mar 2021.

Vancouver:

Espaillat CC. The Evolution of Dusty Disks Around Low-Mass Pre-Main Sequence Stars. [Internet] [Doctoral dissertation]. University of Michigan; 2009. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/2027.42/63766.

Council of Science Editors:

Espaillat CC. The Evolution of Dusty Disks Around Low-Mass Pre-Main Sequence Stars. [Doctoral Dissertation]. University of Michigan; 2009. Available from: http://hdl.handle.net/2027.42/63766


Penn State University

21. Esplin, Taran LeRoy. Observations of Brown Dwarfs at Low Temperatures and Low Masses.

Degree: 2017, Penn State University

 We have contributed to the characterization and discovery of brown dwarfs at low temperatures and low masses. Because the coolest brown dwarfs overlap with giant… (more)

Subjects/Keywords: open clusters and associations: general; astrometry; brown dwarfs; infrared: stars; planets and satellites: atmospheres; solar neighborhood; stars: low-mass; planetary systems; protoplanetary disks; stars: formation; stars: luminosity function; stars: pre-main sequence

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Esplin, T. L. (2017). Observations of Brown Dwarfs at Low Temperatures and Low Masses. (Thesis). Penn State University. Retrieved from https://submit-etda.libraries.psu.edu/catalog/14171tle918

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Esplin, Taran LeRoy. “Observations of Brown Dwarfs at Low Temperatures and Low Masses.” 2017. Thesis, Penn State University. Accessed March 05, 2021. https://submit-etda.libraries.psu.edu/catalog/14171tle918.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Esplin, Taran LeRoy. “Observations of Brown Dwarfs at Low Temperatures and Low Masses.” 2017. Web. 05 Mar 2021.

Vancouver:

Esplin TL. Observations of Brown Dwarfs at Low Temperatures and Low Masses. [Internet] [Thesis]. Penn State University; 2017. [cited 2021 Mar 05]. Available from: https://submit-etda.libraries.psu.edu/catalog/14171tle918.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Esplin TL. Observations of Brown Dwarfs at Low Temperatures and Low Masses. [Thesis]. Penn State University; 2017. Available from: https://submit-etda.libraries.psu.edu/catalog/14171tle918

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


Queens University

22. Grunhut, Jason. Using High-Resolution Spectroscopy To Improve The Determination Of Effective Temperatures OF Pre-Main Sequence Stars .

Degree: Physics, Engineering Physics and Astronomy, 2009, Queens University

 Herbig Ae/Be (HAeBe) stars are the pre-main sequence progenitors of main sequence A and B stars, and are characterized observationally by strong emission in spectral… (more)

Subjects/Keywords: stars ; high-resolution spectroscopy ; pre-main sequence stars ; Herbig stars ; HAeBe stars ; effective temperature

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Grunhut, J. (2009). Using High-Resolution Spectroscopy To Improve The Determination Of Effective Temperatures OF Pre-Main Sequence Stars . (Thesis). Queens University. Retrieved from http://hdl.handle.net/1974/1707

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Grunhut, Jason. “Using High-Resolution Spectroscopy To Improve The Determination Of Effective Temperatures OF Pre-Main Sequence Stars .” 2009. Thesis, Queens University. Accessed March 05, 2021. http://hdl.handle.net/1974/1707.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Grunhut, Jason. “Using High-Resolution Spectroscopy To Improve The Determination Of Effective Temperatures OF Pre-Main Sequence Stars .” 2009. Web. 05 Mar 2021.

Vancouver:

Grunhut J. Using High-Resolution Spectroscopy To Improve The Determination Of Effective Temperatures OF Pre-Main Sequence Stars . [Internet] [Thesis]. Queens University; 2009. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/1974/1707.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Grunhut J. Using High-Resolution Spectroscopy To Improve The Determination Of Effective Temperatures OF Pre-Main Sequence Stars . [Thesis]. Queens University; 2009. Available from: http://hdl.handle.net/1974/1707

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

23. Galli, Phillip Andreas Brenner. Determinação de distâncias cinemáticas de estrelas pré-sequência principal em regiões de formação estelar .

Degree: PhD, Astronomia, 2012, University of São Paulo

Este trabalho tem como objetivo principal a determinação da distância de estrelas pré-sequência principal em regiões de formação estelar próximas. A determinação precisa da distância… (more)

Subjects/Keywords: convergent point; distance; distância; estrelas pré-sequência principal; movimento próprio; moving group; moving group; ponto de convergência; pre-main sequence stars; proper motion

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Galli, P. A. B. (2012). Determinação de distâncias cinemáticas de estrelas pré-sequência principal em regiões de formação estelar . (Doctoral Dissertation). University of São Paulo. Retrieved from http://www.teses.usp.br/teses/disponiveis/14/14131/tde-01042013-194055/ ;

Chicago Manual of Style (16th Edition):

Galli, Phillip Andreas Brenner. “Determinação de distâncias cinemáticas de estrelas pré-sequência principal em regiões de formação estelar .” 2012. Doctoral Dissertation, University of São Paulo. Accessed March 05, 2021. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-01042013-194055/ ;.

MLA Handbook (7th Edition):

Galli, Phillip Andreas Brenner. “Determinação de distâncias cinemáticas de estrelas pré-sequência principal em regiões de formação estelar .” 2012. Web. 05 Mar 2021.

Vancouver:

Galli PAB. Determinação de distâncias cinemáticas de estrelas pré-sequência principal em regiões de formação estelar . [Internet] [Doctoral dissertation]. University of São Paulo; 2012. [cited 2021 Mar 05]. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-01042013-194055/ ;.

Council of Science Editors:

Galli PAB. Determinação de distâncias cinemáticas de estrelas pré-sequência principal em regiões de formação estelar . [Doctoral Dissertation]. University of São Paulo; 2012. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-01042013-194055/ ;


Vanderbilt University

24. Aarnio, Alicia N. The Role of Magnetic Fields in the Pre-Main Sequence Evolution of Solar Type Stars.

Degree: PhD, Physics, 2010, Vanderbilt University

 T Tauri stars, being pre-main sequence and solar mass, tell us what our Sun was like when it was very young. T Tauri stars and… (more)

Subjects/Keywords: stellar flares; solar flares; stellar angular momentum; pre-main sequence stars

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Aarnio, A. N. (2010). The Role of Magnetic Fields in the Pre-Main Sequence Evolution of Solar Type Stars. (Doctoral Dissertation). Vanderbilt University. Retrieved from http://hdl.handle.net/1803/11846

Chicago Manual of Style (16th Edition):

Aarnio, Alicia N. “The Role of Magnetic Fields in the Pre-Main Sequence Evolution of Solar Type Stars.” 2010. Doctoral Dissertation, Vanderbilt University. Accessed March 05, 2021. http://hdl.handle.net/1803/11846.

MLA Handbook (7th Edition):

Aarnio, Alicia N. “The Role of Magnetic Fields in the Pre-Main Sequence Evolution of Solar Type Stars.” 2010. Web. 05 Mar 2021.

Vancouver:

Aarnio AN. The Role of Magnetic Fields in the Pre-Main Sequence Evolution of Solar Type Stars. [Internet] [Doctoral dissertation]. Vanderbilt University; 2010. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/1803/11846.

Council of Science Editors:

Aarnio AN. The Role of Magnetic Fields in the Pre-Main Sequence Evolution of Solar Type Stars. [Doctoral Dissertation]. Vanderbilt University; 2010. Available from: http://hdl.handle.net/1803/11846


University of St. Andrews

25. Gregory, Scott. T Tauri stars : mass accretion and X-ray emission .

Degree: 2007, University of St. Andrews

 I develop the first magnetospheric accretion model to take account of the observed complexity of T Tauri magnetic fields, and the influence of stellar coronae.… (more)

Subjects/Keywords: Star formation; Pre-main sequence stars; Stellar magnetic fields; Stellar coronae

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Gregory, S. (2007). T Tauri stars : mass accretion and X-ray emission . (Thesis). University of St. Andrews. Retrieved from http://hdl.handle.net/10023/336

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Gregory, Scott. “T Tauri stars : mass accretion and X-ray emission .” 2007. Thesis, University of St. Andrews. Accessed March 05, 2021. http://hdl.handle.net/10023/336.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Gregory, Scott. “T Tauri stars : mass accretion and X-ray emission .” 2007. Web. 05 Mar 2021.

Vancouver:

Gregory S. T Tauri stars : mass accretion and X-ray emission . [Internet] [Thesis]. University of St. Andrews; 2007. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/10023/336.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Gregory S. T Tauri stars : mass accretion and X-ray emission . [Thesis]. University of St. Andrews; 2007. Available from: http://hdl.handle.net/10023/336

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

26. Vidotto, Aline de Almeida. Simulações Numéricas Tri-dimensionais de Ventos Magnetizados de Estrelas de Baixa Massa.

Degree: PhD, Astronomia, 2009, University of São Paulo

 O tópico abordado nesta tese é a perda de massa através de ventos coronais magnetizados em estrelas de baixa massa. Ventos estelares têm sido estudados… (more)

Subjects/Keywords: campos magnéticos; estrelas: late-type; estrelas: pre Seqüência Principal; estrelas: ventos; magnetic fields; methods: numerical; métodos: numérico; MHD; outflows; planetas e satélites: geral; planets and satellites: general; stars: late-type; stars: pre-main sequence; stars: winds

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Vidotto, A. d. A. (2009). Simulações Numéricas Tri-dimensionais de Ventos Magnetizados de Estrelas de Baixa Massa. (Doctoral Dissertation). University of São Paulo. Retrieved from http://www.teses.usp.br/teses/disponiveis/14/14131/tde-05082010-071118/ ;

Chicago Manual of Style (16th Edition):

Vidotto, Aline de Almeida. “Simulações Numéricas Tri-dimensionais de Ventos Magnetizados de Estrelas de Baixa Massa.” 2009. Doctoral Dissertation, University of São Paulo. Accessed March 05, 2021. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-05082010-071118/ ;.

MLA Handbook (7th Edition):

Vidotto, Aline de Almeida. “Simulações Numéricas Tri-dimensionais de Ventos Magnetizados de Estrelas de Baixa Massa.” 2009. Web. 05 Mar 2021.

Vancouver:

Vidotto AdA. Simulações Numéricas Tri-dimensionais de Ventos Magnetizados de Estrelas de Baixa Massa. [Internet] [Doctoral dissertation]. University of São Paulo; 2009. [cited 2021 Mar 05]. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-05082010-071118/ ;.

Council of Science Editors:

Vidotto AdA. Simulações Numéricas Tri-dimensionais de Ventos Magnetizados de Estrelas de Baixa Massa. [Doctoral Dissertation]. University of São Paulo; 2009. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-05082010-071118/ ;


Leiden University

27. Lommen, D.J.P. The first steps of planet formation : studying grain growth with millimetre interferometers.

Degree: 2009, Leiden University

 We present Submillimeter-Array (SMA) observations of two embedded young stellar objects, Elias 29 and IRS 63. The masses of the central stars, the discs, and… (more)

Subjects/Keywords: Circumstellar matter; Stars: formation; Stars: planetary systems: protoplanetary discs; Stars: pre-main-sequence; Stars: individual: IRS 63; Stars: individual: Elias 29; Stars: individual: WW Cha; Stars: individual: RU Lup; Stars: individual: CS Cha

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Lommen, D. J. P. (2009). The first steps of planet formation : studying grain growth with millimetre interferometers. (Doctoral Dissertation). Leiden University. Retrieved from http://hdl.handle.net/1887/13752

Chicago Manual of Style (16th Edition):

Lommen, D J P. “The first steps of planet formation : studying grain growth with millimetre interferometers.” 2009. Doctoral Dissertation, Leiden University. Accessed March 05, 2021. http://hdl.handle.net/1887/13752.

MLA Handbook (7th Edition):

Lommen, D J P. “The first steps of planet formation : studying grain growth with millimetre interferometers.” 2009. Web. 05 Mar 2021.

Vancouver:

Lommen DJP. The first steps of planet formation : studying grain growth with millimetre interferometers. [Internet] [Doctoral dissertation]. Leiden University; 2009. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/1887/13752.

Council of Science Editors:

Lommen DJP. The first steps of planet formation : studying grain growth with millimetre interferometers. [Doctoral Dissertation]. Leiden University; 2009. Available from: http://hdl.handle.net/1887/13752

28. Geers, Vincent Carlo. Polycyclic aromatic hydrocarbons in disks around young solar-type stars.

Degree: 2007, Leiden Observatory, Faculty of Science, Leiden University

 In this thesis we study the dust around solar-type young stars. In particular, we focus on one specific species of dust, namely the Polycyclic Aromatic… (more)

Subjects/Keywords: Stars: Pre-main sequence; Stars: planetary systems: protoplanetary disks; Circumstellar matter; Astrochemistry; ISM: molecules; Stars: Pre-main sequence; Stars: planetary systems: protoplanetary disks; Circumstellar matter; Astrochemistry; ISM: molecules

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Geers, V. C. (2007). Polycyclic aromatic hydrocarbons in disks around young solar-type stars. (Doctoral Dissertation). Leiden Observatory, Faculty of Science, Leiden University. Retrieved from http://hdl.handle.net/1887/12414

Chicago Manual of Style (16th Edition):

Geers, Vincent Carlo. “Polycyclic aromatic hydrocarbons in disks around young solar-type stars.” 2007. Doctoral Dissertation, Leiden Observatory, Faculty of Science, Leiden University. Accessed March 05, 2021. http://hdl.handle.net/1887/12414.

MLA Handbook (7th Edition):

Geers, Vincent Carlo. “Polycyclic aromatic hydrocarbons in disks around young solar-type stars.” 2007. Web. 05 Mar 2021.

Vancouver:

Geers VC. Polycyclic aromatic hydrocarbons in disks around young solar-type stars. [Internet] [Doctoral dissertation]. Leiden Observatory, Faculty of Science, Leiden University; 2007. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/1887/12414.

Council of Science Editors:

Geers VC. Polycyclic aromatic hydrocarbons in disks around young solar-type stars. [Doctoral Dissertation]. Leiden Observatory, Faculty of Science, Leiden University; 2007. Available from: http://hdl.handle.net/1887/12414


University of Florida

29. Fleck, Robert Charles, 1949-. Magnetic braking during star formation.

Degree: 1977, University of Florida

Subjects/Keywords: Angular momentum; Braking; Cooling; Cosmic rays; Ionization; Magnetic fields; Magnetism; Magnets; Main sequence stars; Stellar rotation; Astronomy thesis Ph. D; Stars  – Evolution; Stars  – Rotation; Stars, New

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Fleck, Robert Charles, 1. (1977). Magnetic braking during star formation. (Thesis). University of Florida. Retrieved from https://ufdc.ufl.edu/UF00097484

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Fleck, Robert Charles, 1949-. “Magnetic braking during star formation.” 1977. Thesis, University of Florida. Accessed March 05, 2021. https://ufdc.ufl.edu/UF00097484.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Fleck, Robert Charles, 1949-. “Magnetic braking during star formation.” 1977. Web. 05 Mar 2021.

Vancouver:

Fleck, Robert Charles 1. Magnetic braking during star formation. [Internet] [Thesis]. University of Florida; 1977. [cited 2021 Mar 05]. Available from: https://ufdc.ufl.edu/UF00097484.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Fleck, Robert Charles 1. Magnetic braking during star formation. [Thesis]. University of Florida; 1977. Available from: https://ufdc.ufl.edu/UF00097484

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


Universidade Federal de Santa Maria

30. Márcio do Carmo Pinheiro. ESTUDO MULTIBANDA DO CONTEÚDO ESTELAR DE REGIÕES Hii DO HEMISFÉRIO SUL.

Degree: 2012, Universidade Federal de Santa Maria

 We present a multi-wavelength study of the stellar content of 11 optical/infrared Southern Galactic Hii regions with 10 h <(J2000) <−17 h and −65 <(J2000)… (more)

Subjects/Keywords: extinção infravermelho: estrelas; pré-sequência: principal matéria circum-estelar poeira; formação; distâncias; regiões Hii estrelas: estrelas massivas; FISICA; formation; pre-main-sequence circumstellar matter dust; distances; Hii regions stars: early-type; extinction infrared: stars

Record DetailsSimilar RecordsGoogle PlusoneFacebookTwitterCiteULikeMendeleyreddit

APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Pinheiro, M. d. C. (2012). ESTUDO MULTIBANDA DO CONTEÚDO ESTELAR DE REGIÕES Hii DO HEMISFÉRIO SUL. (Thesis). Universidade Federal de Santa Maria. Retrieved from http://coralx.ufsm.br/tede/tde_busca/arquivo.php?codArquivo=5089

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Pinheiro, Márcio do Carmo. “ESTUDO MULTIBANDA DO CONTEÚDO ESTELAR DE REGIÕES Hii DO HEMISFÉRIO SUL.” 2012. Thesis, Universidade Federal de Santa Maria. Accessed March 05, 2021. http://coralx.ufsm.br/tede/tde_busca/arquivo.php?codArquivo=5089.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Pinheiro, Márcio do Carmo. “ESTUDO MULTIBANDA DO CONTEÚDO ESTELAR DE REGIÕES Hii DO HEMISFÉRIO SUL.” 2012. Web. 05 Mar 2021.

Vancouver:

Pinheiro MdC. ESTUDO MULTIBANDA DO CONTEÚDO ESTELAR DE REGIÕES Hii DO HEMISFÉRIO SUL. [Internet] [Thesis]. Universidade Federal de Santa Maria; 2012. [cited 2021 Mar 05]. Available from: http://coralx.ufsm.br/tede/tde_busca/arquivo.php?codArquivo=5089.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Pinheiro MdC. ESTUDO MULTIBANDA DO CONTEÚDO ESTELAR DE REGIÕES Hii DO HEMISFÉRIO SUL. [Thesis]. Universidade Federal de Santa Maria; 2012. Available from: http://coralx.ufsm.br/tede/tde_busca/arquivo.php?codArquivo=5089

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

[1] [2]

.