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You searched for subject:(Stars Evolution). Showing records 1 – 30 of 140 total matches.

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University of Victoria

1. Lyder, David Anthony. Star formation in Camelopardalis: Cam OB1.

Degree: Department of Physics and Astronomy, 2018, University of Victoria

 Star formation in the Cam OB1 region is investigated. Star formation, in general, is considered in terms of three elements: a) the structural relationship between… (more)

Subjects/Keywords: Stars; Evolution

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APA (6th Edition):

Lyder, D. A. (2018). Star formation in Camelopardalis: Cam OB1. (Thesis). University of Victoria. Retrieved from https://dspace.library.uvic.ca//handle/1828/9769

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):

Lyder, David Anthony. “Star formation in Camelopardalis: Cam OB1.” 2018. Thesis, University of Victoria. Accessed March 08, 2021. https://dspace.library.uvic.ca//handle/1828/9769.

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

MLA Handbook (7th Edition):

Lyder, David Anthony. “Star formation in Camelopardalis: Cam OB1.” 2018. Web. 08 Mar 2021.

Vancouver:

Lyder DA. Star formation in Camelopardalis: Cam OB1. [Internet] [Thesis]. University of Victoria; 2018. [cited 2021 Mar 08]. Available from: https://dspace.library.uvic.ca//handle/1828/9769.

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

Council of Science Editors:

Lyder DA. Star formation in Camelopardalis: Cam OB1. [Thesis]. University of Victoria; 2018. Available from: https://dspace.library.uvic.ca//handle/1828/9769

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


University of Hong Kong

2. Wong, Ka-tat. SiO-emitting condensations throughout the envelope of the yellow hypergiant IRC+10420.

Degree: 2013, University of Hong Kong

 IRC+10420 is a massive (> 20M☉), very luminous (> 〖10〗6L☉) star that is in the rare phase of evolution from the red supergiant to the… (more)

Subjects/Keywords: Stars - Evolution

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APA (6th Edition):

Wong, K. (2013). SiO-emitting condensations throughout the envelope of the yellow hypergiant IRC+10420. (Thesis). University of Hong Kong. Retrieved from http://hdl.handle.net/10722/195970

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):

Wong, Ka-tat. “SiO-emitting condensations throughout the envelope of the yellow hypergiant IRC+10420.” 2013. Thesis, University of Hong Kong. Accessed March 08, 2021. http://hdl.handle.net/10722/195970.

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

MLA Handbook (7th Edition):

Wong, Ka-tat. “SiO-emitting condensations throughout the envelope of the yellow hypergiant IRC+10420.” 2013. Web. 08 Mar 2021.

Vancouver:

Wong K. SiO-emitting condensations throughout the envelope of the yellow hypergiant IRC+10420. [Internet] [Thesis]. University of Hong Kong; 2013. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/10722/195970.

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

Council of Science Editors:

Wong K. SiO-emitting condensations throughout the envelope of the yellow hypergiant IRC+10420. [Thesis]. University of Hong Kong; 2013. Available from: http://hdl.handle.net/10722/195970

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


University of Arizona

3. Adams, Mark Thomas. AN OBSERVATIONAL STUDY OF LOW-MASS STAR FORMATION IN NGC 2264 .

Degree: 1981, University of Arizona

 The history of an actively star-forming region, containing the young, open cluster NGC 2264, is examined in this thesis using UBVRIHα photographic plate material. After… (more)

Subjects/Keywords: Stars  – Evolution.

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APA (6th Edition):

Adams, M. T. (1981). AN OBSERVATIONAL STUDY OF LOW-MASS STAR FORMATION IN NGC 2264 . (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/282033

Chicago Manual of Style (16th Edition):

Adams, Mark Thomas. “AN OBSERVATIONAL STUDY OF LOW-MASS STAR FORMATION IN NGC 2264 .” 1981. Doctoral Dissertation, University of Arizona. Accessed March 08, 2021. http://hdl.handle.net/10150/282033.

MLA Handbook (7th Edition):

Adams, Mark Thomas. “AN OBSERVATIONAL STUDY OF LOW-MASS STAR FORMATION IN NGC 2264 .” 1981. Web. 08 Mar 2021.

Vancouver:

Adams MT. AN OBSERVATIONAL STUDY OF LOW-MASS STAR FORMATION IN NGC 2264 . [Internet] [Doctoral dissertation]. University of Arizona; 1981. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/10150/282033.

Council of Science Editors:

Adams MT. AN OBSERVATIONAL STUDY OF LOW-MASS STAR FORMATION IN NGC 2264 . [Doctoral Dissertation]. University of Arizona; 1981. Available from: http://hdl.handle.net/10150/282033


Vilnius University

4. Puzeras, Eduardas. Evoliuciniai cheminės sudėties pokyčiai helį centre deginančių žvaigždžių atmosferose.

Degree: PhD, Physics, 2011, Vilnius University

Šiuolaikiniai astronominiai stebėjimai leidžia įtarti, kad „standartinis“ žvaigždžių evoliucijos modelis yra nepilnas ir turi būti patikslintas, įvedant „papildomą“ maišymąsi. Disertacija yra skirta Galaktikos raudonosios sankaupos… (more)

Subjects/Keywords: Žvaigždės; Žvaigždžių cheminė sudėtis; Žvaigždžių evoliucija; Stars; Abundances-stars; Evolution-stars

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APA (6th Edition):

Puzeras, Eduardas. (2011). Evoliuciniai cheminės sudėties pokyčiai helį centre deginančių žvaigždžių atmosferose. (Doctoral Dissertation). Vilnius University. Retrieved from http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2011~D_20111102_110809-17295 ;

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete

Chicago Manual of Style (16th Edition):

Puzeras, Eduardas. “Evoliuciniai cheminės sudėties pokyčiai helį centre deginančių žvaigždžių atmosferose.” 2011. Doctoral Dissertation, Vilnius University. Accessed March 08, 2021. http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2011~D_20111102_110809-17295 ;.

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete

MLA Handbook (7th Edition):

Puzeras, Eduardas. “Evoliuciniai cheminės sudėties pokyčiai helį centre deginančių žvaigždžių atmosferose.” 2011. Web. 08 Mar 2021.

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete

Vancouver:

Puzeras, Eduardas. Evoliuciniai cheminės sudėties pokyčiai helį centre deginančių žvaigždžių atmosferose. [Internet] [Doctoral dissertation]. Vilnius University; 2011. [cited 2021 Mar 08]. Available from: http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2011~D_20111102_110809-17295 ;.

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete

Council of Science Editors:

Puzeras, Eduardas. Evoliuciniai cheminės sudėties pokyčiai helį centre deginančių žvaigždžių atmosferose. [Doctoral Dissertation]. Vilnius University; 2011. Available from: http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2011~D_20111102_110809-17295 ;

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete


Vilnius University

5. Puzeras, Eduardas. Evolutionary effects in helium core burning star atmospheres.

Degree: Dissertation, Physics, 2011, Vilnius University

Modern observations provide evidences that the ‘standard’ stellar evolution model is incomplete and should take into account ‘extra’-mixing processes. This dissertation is dedicated to an… (more)

Subjects/Keywords: Stars; Abundances-stars; Evolution-stars; Žvaigždės; Žvaigždžių cheminė sudėtis; Žvaigždžių evoliucija

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APA (6th Edition):

Puzeras, Eduardas. (2011). Evolutionary effects in helium core burning star atmospheres. (Doctoral Dissertation). Vilnius University. Retrieved from http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2011~D_20111102_110919-19082 ;

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete

Chicago Manual of Style (16th Edition):

Puzeras, Eduardas. “Evolutionary effects in helium core burning star atmospheres.” 2011. Doctoral Dissertation, Vilnius University. Accessed March 08, 2021. http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2011~D_20111102_110919-19082 ;.

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete

MLA Handbook (7th Edition):

Puzeras, Eduardas. “Evolutionary effects in helium core burning star atmospheres.” 2011. Web. 08 Mar 2021.

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete

Vancouver:

Puzeras, Eduardas. Evolutionary effects in helium core burning star atmospheres. [Internet] [Doctoral dissertation]. Vilnius University; 2011. [cited 2021 Mar 08]. Available from: http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2011~D_20111102_110919-19082 ;.

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete

Council of Science Editors:

Puzeras, Eduardas. Evolutionary effects in helium core burning star atmospheres. [Doctoral Dissertation]. Vilnius University; 2011. Available from: http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2011~D_20111102_110919-19082 ;

Note: this citation may be lacking information needed for this citation format:
Author name may be incomplete


Columbia University

6. Andrews, Jeffrey. Double White Dwarfs as Probes of Single and Binary Star Evolution.

Degree: 2016, Columbia University

 As the endpoints of stars less massive than roughly eight solar masses, the population of Galactic white dwarfs (WD) contain information about complex stellar evolution(more)

Subjects/Keywords: White dwarf stars; Binary stars; Stars – Evolution; Astronomy; Astrophysics

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APA (6th Edition):

Andrews, J. (2016). Double White Dwarfs as Probes of Single and Binary Star Evolution. (Doctoral Dissertation). Columbia University. Retrieved from https://doi.org/10.7916/D8VH5NQ4

Chicago Manual of Style (16th Edition):

Andrews, Jeffrey. “Double White Dwarfs as Probes of Single and Binary Star Evolution.” 2016. Doctoral Dissertation, Columbia University. Accessed March 08, 2021. https://doi.org/10.7916/D8VH5NQ4.

MLA Handbook (7th Edition):

Andrews, Jeffrey. “Double White Dwarfs as Probes of Single and Binary Star Evolution.” 2016. Web. 08 Mar 2021.

Vancouver:

Andrews J. Double White Dwarfs as Probes of Single and Binary Star Evolution. [Internet] [Doctoral dissertation]. Columbia University; 2016. [cited 2021 Mar 08]. Available from: https://doi.org/10.7916/D8VH5NQ4.

Council of Science Editors:

Andrews J. Double White Dwarfs as Probes of Single and Binary Star Evolution. [Doctoral Dissertation]. Columbia University; 2016. Available from: https://doi.org/10.7916/D8VH5NQ4


Michigan State University

7. Crosby, Brian David. Semi-analytic modeling of stellar populations in astrophysical simulations.

Degree: 2016, Michigan State University

Thesis Ph. D. Michigan State University. Astrophysics and Astronomy 2016

Understanding galaxy formation is an enduring questions in astrophysics. Galaxies are systems rich in interesting… (more)

Subjects/Keywords: Stars – Populations – Simulation methods; Stars – Evolution; Galaxies – Evolution; Astrophysics

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APA (6th Edition):

Crosby, B. D. (2016). Semi-analytic modeling of stellar populations in astrophysical simulations. (Thesis). Michigan State University. Retrieved from http://etd.lib.msu.edu/islandora/object/etd:4360

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):

Crosby, Brian David. “Semi-analytic modeling of stellar populations in astrophysical simulations.” 2016. Thesis, Michigan State University. Accessed March 08, 2021. http://etd.lib.msu.edu/islandora/object/etd:4360.

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

MLA Handbook (7th Edition):

Crosby, Brian David. “Semi-analytic modeling of stellar populations in astrophysical simulations.” 2016. Web. 08 Mar 2021.

Vancouver:

Crosby BD. Semi-analytic modeling of stellar populations in astrophysical simulations. [Internet] [Thesis]. Michigan State University; 2016. [cited 2021 Mar 08]. Available from: http://etd.lib.msu.edu/islandora/object/etd:4360.

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

Council of Science Editors:

Crosby BD. Semi-analytic modeling of stellar populations in astrophysical simulations. [Thesis]. Michigan State University; 2016. Available from: http://etd.lib.msu.edu/islandora/object/etd:4360

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


Universiteit Utrecht

8. Bonačić Marinović, A.A. Nucleosynthesis and evolution of AGB stars in binary systems.

Degree: 2007, Universiteit Utrecht

 Thermally-pulsating asymptotic giant branch (TP-AGB) stars are hundreds of times larger and several tens of thousand times more luminous than than the Sun. They are… (more)

Subjects/Keywords: Natuur- en Sterrenkunde; stars: AGB and post-AGB; stars; abundances; nucleosynthesis; stars: binary; stars: evolution; stars: Sirius

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APA (6th Edition):

Bonačić Marinović, A. A. (2007). Nucleosynthesis and evolution of AGB stars in binary systems. (Doctoral Dissertation). Universiteit Utrecht. Retrieved from http://dspace.library.uu.nl:8080/handle/1874/23521

Chicago Manual of Style (16th Edition):

Bonačić Marinović, A A. “Nucleosynthesis and evolution of AGB stars in binary systems.” 2007. Doctoral Dissertation, Universiteit Utrecht. Accessed March 08, 2021. http://dspace.library.uu.nl:8080/handle/1874/23521.

MLA Handbook (7th Edition):

Bonačić Marinović, A A. “Nucleosynthesis and evolution of AGB stars in binary systems.” 2007. Web. 08 Mar 2021.

Vancouver:

Bonačić Marinović AA. Nucleosynthesis and evolution of AGB stars in binary systems. [Internet] [Doctoral dissertation]. Universiteit Utrecht; 2007. [cited 2021 Mar 08]. Available from: http://dspace.library.uu.nl:8080/handle/1874/23521.

Council of Science Editors:

Bonačić Marinović AA. Nucleosynthesis and evolution of AGB stars in binary systems. [Doctoral Dissertation]. Universiteit Utrecht; 2007. Available from: http://dspace.library.uu.nl:8080/handle/1874/23521

9. BYRNE, CONOR MICHAEL. Atomic Diffusion and Pulsation in Post-Common-Envelope Binary Stars.

Degree: School of Physics. Discipline of Physics, 2020, Trinity College Dublin

 I study the evolution of peculiar low-mass, evolved stars. Two groups of interest are the core-helium-burning hot subdwarfs and the shell-hydrogen-burning low-mass pre-white dwarfs. Stars(more)

Subjects/Keywords: subdwarfs; white dwarfs; stars evolution; diffusion; stars horizontal branch; stars oscillations; atomic processes; stars chemically peculiar; stars abundances

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APA (6th Edition):

BYRNE, C. M. (2020). Atomic Diffusion and Pulsation in Post-Common-Envelope Binary Stars. (Thesis). Trinity College Dublin. Retrieved from http://hdl.handle.net/2262/92683

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):

BYRNE, CONOR MICHAEL. “Atomic Diffusion and Pulsation in Post-Common-Envelope Binary Stars.” 2020. Thesis, Trinity College Dublin. Accessed March 08, 2021. http://hdl.handle.net/2262/92683.

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

MLA Handbook (7th Edition):

BYRNE, CONOR MICHAEL. “Atomic Diffusion and Pulsation in Post-Common-Envelope Binary Stars.” 2020. Web. 08 Mar 2021.

Vancouver:

BYRNE CM. Atomic Diffusion and Pulsation in Post-Common-Envelope Binary Stars. [Internet] [Thesis]. Trinity College Dublin; 2020. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/2262/92683.

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

Council of Science Editors:

BYRNE CM. Atomic Diffusion and Pulsation in Post-Common-Envelope Binary Stars. [Thesis]. Trinity College Dublin; 2020. Available from: http://hdl.handle.net/2262/92683

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


University of Hawaii – Manoa

10. Dahm, Scott E. The evolution of young clusters.

Degree: PhD, 2009, University of Hawaii – Manoa

Electronic reproduction.

Also available by subscription via World Wide Web

xvii, 261 leaves, bound ill. (some col.) 29 cm

Subjects/Keywords: Stars  – Clusters; Stars  – Evolution; Stars  – Formation

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APA (6th Edition):

Dahm, S. E. (2009). The evolution of young clusters. (Doctoral Dissertation). University of Hawaii – Manoa. Retrieved from http://hdl.handle.net/10125/12105

Chicago Manual of Style (16th Edition):

Dahm, Scott E. “The evolution of young clusters.” 2009. Doctoral Dissertation, University of Hawaii – Manoa. Accessed March 08, 2021. http://hdl.handle.net/10125/12105.

MLA Handbook (7th Edition):

Dahm, Scott E. “The evolution of young clusters.” 2009. Web. 08 Mar 2021.

Vancouver:

Dahm SE. The evolution of young clusters. [Internet] [Doctoral dissertation]. University of Hawaii – Manoa; 2009. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/10125/12105.

Council of Science Editors:

Dahm SE. The evolution of young clusters. [Doctoral Dissertation]. University of Hawaii – Manoa; 2009. Available from: http://hdl.handle.net/10125/12105

11. Weston, Simon. Post asymptotic giant branch and central stars of planetary nebulae in the Galactic halo.

Degree: PhD, 2012, University of Hertfordshire

 Post asymptotic giant branch (post-AGB) stars, central stars of planetary nebulae (CSPNe) and planetary nebulae (PNe) are important phases of stellar evolution as the material… (more)

Subjects/Keywords: 523.8; stars: evolution; stars: AGB and post-AGB; Galaxy: halo

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APA (6th Edition):

Weston, S. (2012). Post asymptotic giant branch and central stars of planetary nebulae in the Galactic halo. (Doctoral Dissertation). University of Hertfordshire. Retrieved from http://hdl.handle.net/2299/9042

Chicago Manual of Style (16th Edition):

Weston, Simon. “Post asymptotic giant branch and central stars of planetary nebulae in the Galactic halo.” 2012. Doctoral Dissertation, University of Hertfordshire. Accessed March 08, 2021. http://hdl.handle.net/2299/9042.

MLA Handbook (7th Edition):

Weston, Simon. “Post asymptotic giant branch and central stars of planetary nebulae in the Galactic halo.” 2012. Web. 08 Mar 2021.

Vancouver:

Weston S. Post asymptotic giant branch and central stars of planetary nebulae in the Galactic halo. [Internet] [Doctoral dissertation]. University of Hertfordshire; 2012. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/2299/9042.

Council of Science Editors:

Weston S. Post asymptotic giant branch and central stars of planetary nebulae in the Galactic halo. [Doctoral Dissertation]. University of Hertfordshire; 2012. Available from: http://hdl.handle.net/2299/9042


University of Minnesota

12. Grammer, Skyler. The massive Star Population in M101.

Degree: PhD, 2014, University of Minnesota

 An increasing number of non-terminal giant eruptions are being observed by modern supernova and transient surveys. Very little is known about the origin of these… (more)

Subjects/Keywords: Galaxies; Massive Stars; Stellar evolution; Astrophysics

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APA (6th Edition):

Grammer, S. (2014). The massive Star Population in M101. (Doctoral Dissertation). University of Minnesota. Retrieved from http://hdl.handle.net/11299/167865

Chicago Manual of Style (16th Edition):

Grammer, Skyler. “The massive Star Population in M101.” 2014. Doctoral Dissertation, University of Minnesota. Accessed March 08, 2021. http://hdl.handle.net/11299/167865.

MLA Handbook (7th Edition):

Grammer, Skyler. “The massive Star Population in M101.” 2014. Web. 08 Mar 2021.

Vancouver:

Grammer S. The massive Star Population in M101. [Internet] [Doctoral dissertation]. University of Minnesota; 2014. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/11299/167865.

Council of Science Editors:

Grammer S. The massive Star Population in M101. [Doctoral Dissertation]. University of Minnesota; 2014. Available from: http://hdl.handle.net/11299/167865


University of Arizona

13. Vrba, Frederick John, 1949-. THE MAGNETIC FIELD STRUCTURE AND EMBEDDED STELLAR POPULATION OF DARK CLOUD COMPLEXES .

Degree: 1976, University of Arizona

Subjects/Keywords: Nebulae.; Stars  – Evolution.

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APA (6th Edition):

Vrba, Frederick John, 1. (1976). THE MAGNETIC FIELD STRUCTURE AND EMBEDDED STELLAR POPULATION OF DARK CLOUD COMPLEXES . (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/289404

Chicago Manual of Style (16th Edition):

Vrba, Frederick John, 1949-. “THE MAGNETIC FIELD STRUCTURE AND EMBEDDED STELLAR POPULATION OF DARK CLOUD COMPLEXES .” 1976. Doctoral Dissertation, University of Arizona. Accessed March 08, 2021. http://hdl.handle.net/10150/289404.

MLA Handbook (7th Edition):

Vrba, Frederick John, 1949-. “THE MAGNETIC FIELD STRUCTURE AND EMBEDDED STELLAR POPULATION OF DARK CLOUD COMPLEXES .” 1976. Web. 08 Mar 2021.

Vancouver:

Vrba, Frederick John 1. THE MAGNETIC FIELD STRUCTURE AND EMBEDDED STELLAR POPULATION OF DARK CLOUD COMPLEXES . [Internet] [Doctoral dissertation]. University of Arizona; 1976. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/10150/289404.

Council of Science Editors:

Vrba, Frederick John 1. THE MAGNETIC FIELD STRUCTURE AND EMBEDDED STELLAR POPULATION OF DARK CLOUD COMPLEXES . [Doctoral Dissertation]. University of Arizona; 1976. Available from: http://hdl.handle.net/10150/289404


University of Arizona

14. Jensen, Eric Bruce, 1948-. THE NATURE OF HEAVY-ELEMENT ABUNDANCE GRADIENTS IN GALAXIES .

Degree: 1977, University of Arizona

Subjects/Keywords: Stars  – Evolution.; Galaxies.

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APA (6th Edition):

Jensen, Eric Bruce, 1. (1977). THE NATURE OF HEAVY-ELEMENT ABUNDANCE GRADIENTS IN GALAXIES . (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/289539

Chicago Manual of Style (16th Edition):

Jensen, Eric Bruce, 1948-. “THE NATURE OF HEAVY-ELEMENT ABUNDANCE GRADIENTS IN GALAXIES .” 1977. Doctoral Dissertation, University of Arizona. Accessed March 08, 2021. http://hdl.handle.net/10150/289539.

MLA Handbook (7th Edition):

Jensen, Eric Bruce, 1948-. “THE NATURE OF HEAVY-ELEMENT ABUNDANCE GRADIENTS IN GALAXIES .” 1977. Web. 08 Mar 2021.

Vancouver:

Jensen, Eric Bruce 1. THE NATURE OF HEAVY-ELEMENT ABUNDANCE GRADIENTS IN GALAXIES . [Internet] [Doctoral dissertation]. University of Arizona; 1977. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/10150/289539.

Council of Science Editors:

Jensen, Eric Bruce 1. THE NATURE OF HEAVY-ELEMENT ABUNDANCE GRADIENTS IN GALAXIES . [Doctoral Dissertation]. University of Arizona; 1977. Available from: http://hdl.handle.net/10150/289539


University of Arizona

15. Lowenthal, James Daniel. Line emission from galaxies at high redshift.

Degree: 1991, University of Arizona

 The results of a multi-faceted search for spectral line emission from galaxies at high redshift are presented. Deep two-dimensional spectra of four blank sky fields… (more)

Subjects/Keywords: Stars  – Evolution; Galaxies.

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APA (6th Edition):

Lowenthal, J. D. (1991). Line emission from galaxies at high redshift. (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/185621

Chicago Manual of Style (16th Edition):

Lowenthal, James Daniel. “Line emission from galaxies at high redshift. ” 1991. Doctoral Dissertation, University of Arizona. Accessed March 08, 2021. http://hdl.handle.net/10150/185621.

MLA Handbook (7th Edition):

Lowenthal, James Daniel. “Line emission from galaxies at high redshift. ” 1991. Web. 08 Mar 2021.

Vancouver:

Lowenthal JD. Line emission from galaxies at high redshift. [Internet] [Doctoral dissertation]. University of Arizona; 1991. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/10150/185621.

Council of Science Editors:

Lowenthal JD. Line emission from galaxies at high redshift. [Doctoral Dissertation]. University of Arizona; 1991. Available from: http://hdl.handle.net/10150/185621


University of Victoria

16. Clarkson, Ondrea. The first stars and the convective-reactive regime.

Degree: Department of Physics and Astronomy, 2021, University of Victoria

 Due to their initially metal-free composition, the fi rst stars in the Universe, which are termed Population III (Pop III) stars, were fundamentally different than… (more)

Subjects/Keywords: Stars; Population III; Stellar Evolution; Nucleosynthesis

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APA (6th Edition):

Clarkson, O. (2021). The first stars and the convective-reactive regime. (Thesis). University of Victoria. Retrieved from http://hdl.handle.net/1828/12548

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):

Clarkson, Ondrea. “The first stars and the convective-reactive regime.” 2021. Thesis, University of Victoria. Accessed March 08, 2021. http://hdl.handle.net/1828/12548.

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

MLA Handbook (7th Edition):

Clarkson, Ondrea. “The first stars and the convective-reactive regime.” 2021. Web. 08 Mar 2021.

Vancouver:

Clarkson O. The first stars and the convective-reactive regime. [Internet] [Thesis]. University of Victoria; 2021. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/1828/12548.

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

Council of Science Editors:

Clarkson O. The first stars and the convective-reactive regime. [Thesis]. University of Victoria; 2021. Available from: http://hdl.handle.net/1828/12548

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

17. Matson, Rachel A. Fundamental Parameters of Eclipsing Binaries in the Kepler Field of View.

Degree: PhD, Physics and Astronomy, 2016, Georgia State University

  Accurate knowledge of stellar parameters such as mass, radius, effective temperature, and composition inform our understanding of stellar evolution and constrain theoretical models. Binaries… (more)

Subjects/Keywords: astronomy; binaries; binaries: eclipsing; binaries: spectroscopic; stars: fundamental parameters; stars: evolution; stars: individual (KIC 5738698); stars: individual (KOI-81)

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APA (6th Edition):

Matson, R. A. (2016). Fundamental Parameters of Eclipsing Binaries in the Kepler Field of View. (Doctoral Dissertation). Georgia State University. Retrieved from https://scholarworks.gsu.edu/phy_astr_diss/91

Chicago Manual of Style (16th Edition):

Matson, Rachel A. “Fundamental Parameters of Eclipsing Binaries in the Kepler Field of View.” 2016. Doctoral Dissertation, Georgia State University. Accessed March 08, 2021. https://scholarworks.gsu.edu/phy_astr_diss/91.

MLA Handbook (7th Edition):

Matson, Rachel A. “Fundamental Parameters of Eclipsing Binaries in the Kepler Field of View.” 2016. Web. 08 Mar 2021.

Vancouver:

Matson RA. Fundamental Parameters of Eclipsing Binaries in the Kepler Field of View. [Internet] [Doctoral dissertation]. Georgia State University; 2016. [cited 2021 Mar 08]. Available from: https://scholarworks.gsu.edu/phy_astr_diss/91.

Council of Science Editors:

Matson RA. Fundamental Parameters of Eclipsing Binaries in the Kepler Field of View. [Doctoral Dissertation]. Georgia State University; 2016. Available from: https://scholarworks.gsu.edu/phy_astr_diss/91


Columbia University

18. Emerick, Andrew James. Stellar Feedback and Chemical Evolution In Dwarf Galaxies.

Degree: 2019, Columbia University

 Motivated by the desire to investigate two of the largest outstanding problems in galactic evolution  – stellar feedback and galactic chemical evolution  – we develop… (more)

Subjects/Keywords: Astronomy; Astrophysics; Galaxies – Evolution; Molecular evolution; Stars – Formation

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APA (6th Edition):

Emerick, A. J. (2019). Stellar Feedback and Chemical Evolution In Dwarf Galaxies. (Doctoral Dissertation). Columbia University. Retrieved from https://doi.org/10.7916/d8-29kz-8d92

Chicago Manual of Style (16th Edition):

Emerick, Andrew James. “Stellar Feedback and Chemical Evolution In Dwarf Galaxies.” 2019. Doctoral Dissertation, Columbia University. Accessed March 08, 2021. https://doi.org/10.7916/d8-29kz-8d92.

MLA Handbook (7th Edition):

Emerick, Andrew James. “Stellar Feedback and Chemical Evolution In Dwarf Galaxies.” 2019. Web. 08 Mar 2021.

Vancouver:

Emerick AJ. Stellar Feedback and Chemical Evolution In Dwarf Galaxies. [Internet] [Doctoral dissertation]. Columbia University; 2019. [cited 2021 Mar 08]. Available from: https://doi.org/10.7916/d8-29kz-8d92.

Council of Science Editors:

Emerick AJ. Stellar Feedback and Chemical Evolution In Dwarf Galaxies. [Doctoral Dissertation]. Columbia University; 2019. Available from: https://doi.org/10.7916/d8-29kz-8d92

19. Titarenko, Anastasia. Indicateurs chimiques d’âge stellaire à l’ère de Gaia : Stellar chemical clocks in the Gaia era.

Degree: Docteur es, Sciences de la planète et de l'univers, 2018, Université Côte d'Azur (ComUE)

 Les étoiles enregistrent le passé dans leurs âges, leurs compositions chimiques et leur cinématique. Elles peuvent fournir des contraintes détaillées sur les premières époques de… (more)

Subjects/Keywords: Étoiles : âges; Étoiles : abondances; Étoiles : évolution; Étoiles : paramètres fondamentaux; Galaxie : disque; Galaxie : évolution; Stars: ages; Stars: abundances; Stars: evolution; Stars: fundamental parameters; Galaxy: disk; Galaxy: evolution

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APA (6th Edition):

Titarenko, A. (2018). Indicateurs chimiques d’âge stellaire à l’ère de Gaia : Stellar chemical clocks in the Gaia era. (Doctoral Dissertation). Université Côte d'Azur (ComUE). Retrieved from http://www.theses.fr/2018AZUR4065

Chicago Manual of Style (16th Edition):

Titarenko, Anastasia. “Indicateurs chimiques d’âge stellaire à l’ère de Gaia : Stellar chemical clocks in the Gaia era.” 2018. Doctoral Dissertation, Université Côte d'Azur (ComUE). Accessed March 08, 2021. http://www.theses.fr/2018AZUR4065.

MLA Handbook (7th Edition):

Titarenko, Anastasia. “Indicateurs chimiques d’âge stellaire à l’ère de Gaia : Stellar chemical clocks in the Gaia era.” 2018. Web. 08 Mar 2021.

Vancouver:

Titarenko A. Indicateurs chimiques d’âge stellaire à l’ère de Gaia : Stellar chemical clocks in the Gaia era. [Internet] [Doctoral dissertation]. Université Côte d'Azur (ComUE); 2018. [cited 2021 Mar 08]. Available from: http://www.theses.fr/2018AZUR4065.

Council of Science Editors:

Titarenko A. Indicateurs chimiques d’âge stellaire à l’ère de Gaia : Stellar chemical clocks in the Gaia era. [Doctoral Dissertation]. Université Côte d'Azur (ComUE); 2018. Available from: http://www.theses.fr/2018AZUR4065


University of Texas – Austin

20. Bergmann, Marcel Peter. Galaxy evolution: the relationship between structure, star formation, and environment.

Degree: PhD, Astronomy, 2002, University of Texas – Austin

 I have conducted two separate observational tests of the current theoretical paradigm for galaxy formation and evolution, hierarchical galaxy formation in a Cold Dark Matter… (more)

Subjects/Keywords: Galaxies – Evolution; Stars – Formation; Stars – Structure

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APA (6th Edition):

Bergmann, M. P. (2002). Galaxy evolution: the relationship between structure, star formation, and environment. (Doctoral Dissertation). University of Texas – Austin. Retrieved from http://hdl.handle.net/2152/457

Chicago Manual of Style (16th Edition):

Bergmann, Marcel Peter. “Galaxy evolution: the relationship between structure, star formation, and environment.” 2002. Doctoral Dissertation, University of Texas – Austin. Accessed March 08, 2021. http://hdl.handle.net/2152/457.

MLA Handbook (7th Edition):

Bergmann, Marcel Peter. “Galaxy evolution: the relationship between structure, star formation, and environment.” 2002. Web. 08 Mar 2021.

Vancouver:

Bergmann MP. Galaxy evolution: the relationship between structure, star formation, and environment. [Internet] [Doctoral dissertation]. University of Texas – Austin; 2002. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/2152/457.

Council of Science Editors:

Bergmann MP. Galaxy evolution: the relationship between structure, star formation, and environment. [Doctoral Dissertation]. University of Texas – Austin; 2002. Available from: http://hdl.handle.net/2152/457

21. André, Quentin. Ondes gravito-inertielles dans les étoiles et les planètes géantes : propagation, dissipation et échanges de moment cinétique : Gravito-inertial waves in stars and giant planets : propagation, dissipation and angular momentum transport.

Degree: Docteur es, Physique. Astronomie et astrophysique, 2019, Université de Paris (2019-....)

 Les ondes internes gravito-inertielles sont des ondes se propageant dans les milieux fluides stablement stratifiés en rotation. Leurs forces de rappel sont la poussée d'Archimède… (more)

Subjects/Keywords: Interactions de marées; Hydrodynamics; Modelisation; Numerical simulation; Waves; Convection; Giant planets; Tides; Stars  – Rotation; Stars  – Evolution; Massive stars

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APA (6th Edition):

André, Q. (2019). Ondes gravito-inertielles dans les étoiles et les planètes géantes : propagation, dissipation et échanges de moment cinétique : Gravito-inertial waves in stars and giant planets : propagation, dissipation and angular momentum transport. (Doctoral Dissertation). Université de Paris (2019-....). Retrieved from http://www.theses.fr/2019UNIP7073

Chicago Manual of Style (16th Edition):

André, Quentin. “Ondes gravito-inertielles dans les étoiles et les planètes géantes : propagation, dissipation et échanges de moment cinétique : Gravito-inertial waves in stars and giant planets : propagation, dissipation and angular momentum transport.” 2019. Doctoral Dissertation, Université de Paris (2019-....). Accessed March 08, 2021. http://www.theses.fr/2019UNIP7073.

MLA Handbook (7th Edition):

André, Quentin. “Ondes gravito-inertielles dans les étoiles et les planètes géantes : propagation, dissipation et échanges de moment cinétique : Gravito-inertial waves in stars and giant planets : propagation, dissipation and angular momentum transport.” 2019. Web. 08 Mar 2021.

Vancouver:

André Q. Ondes gravito-inertielles dans les étoiles et les planètes géantes : propagation, dissipation et échanges de moment cinétique : Gravito-inertial waves in stars and giant planets : propagation, dissipation and angular momentum transport. [Internet] [Doctoral dissertation]. Université de Paris (2019-....); 2019. [cited 2021 Mar 08]. Available from: http://www.theses.fr/2019UNIP7073.

Council of Science Editors:

André Q. Ondes gravito-inertielles dans les étoiles et les planètes géantes : propagation, dissipation et échanges de moment cinétique : Gravito-inertial waves in stars and giant planets : propagation, dissipation and angular momentum transport. [Doctoral Dissertation]. Université de Paris (2019-....); 2019. Available from: http://www.theses.fr/2019UNIP7073


University of Arizona

22. COOK, KEM HOLLAND. ASYMPTOTIC GIANT BRANCH POPULATIONS IN COMPOSITE STELLAR SYSTEMS.

Degree: 1987, University of Arizona

 This dissertation presents a technique for the identification and classification of late-type stars and for the estimation of M star metallicities. The technique uses broad-band,… (more)

Subjects/Keywords: Stars  – Classification.; Stars  – Evolution.; Cool stars  – Classification.; Astronomy  – Observations.

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APA (6th Edition):

COOK, K. H. (1987). ASYMPTOTIC GIANT BRANCH POPULATIONS IN COMPOSITE STELLAR SYSTEMS. (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/184208

Chicago Manual of Style (16th Edition):

COOK, KEM HOLLAND. “ASYMPTOTIC GIANT BRANCH POPULATIONS IN COMPOSITE STELLAR SYSTEMS. ” 1987. Doctoral Dissertation, University of Arizona. Accessed March 08, 2021. http://hdl.handle.net/10150/184208.

MLA Handbook (7th Edition):

COOK, KEM HOLLAND. “ASYMPTOTIC GIANT BRANCH POPULATIONS IN COMPOSITE STELLAR SYSTEMS. ” 1987. Web. 08 Mar 2021.

Vancouver:

COOK KH. ASYMPTOTIC GIANT BRANCH POPULATIONS IN COMPOSITE STELLAR SYSTEMS. [Internet] [Doctoral dissertation]. University of Arizona; 1987. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/10150/184208.

Council of Science Editors:

COOK KH. ASYMPTOTIC GIANT BRANCH POPULATIONS IN COMPOSITE STELLAR SYSTEMS. [Doctoral Dissertation]. University of Arizona; 1987. Available from: http://hdl.handle.net/10150/184208


York University

23. Moore, Keavin Matthew. Tatooine's Future: Dynamical Evolution of Planets Orbiting Two Stars.

Degree: MSc -MS, Physics And Astronomy, 2018, York University

 Science fiction has long teased our imaginations with tales of planets with two suns. How these planets form and evolve, and their survival prospects, are… (more)

Subjects/Keywords: Astronomy; Astronomy; Astrophysics; Planets; Exoplanets; Extra-solar planets; Circumbinary planets; Stars; Binary stars; Close binary stars; Stellar evolution; Common envelope; Survival; Dynamical evolution; Orbital evolution; Tatooine; Suns

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APA (6th Edition):

Moore, K. M. (2018). Tatooine's Future: Dynamical Evolution of Planets Orbiting Two Stars. (Masters Thesis). York University. Retrieved from http://hdl.handle.net/10315/34393

Chicago Manual of Style (16th Edition):

Moore, Keavin Matthew. “Tatooine's Future: Dynamical Evolution of Planets Orbiting Two Stars.” 2018. Masters Thesis, York University. Accessed March 08, 2021. http://hdl.handle.net/10315/34393.

MLA Handbook (7th Edition):

Moore, Keavin Matthew. “Tatooine's Future: Dynamical Evolution of Planets Orbiting Two Stars.” 2018. Web. 08 Mar 2021.

Vancouver:

Moore KM. Tatooine's Future: Dynamical Evolution of Planets Orbiting Two Stars. [Internet] [Masters thesis]. York University; 2018. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/10315/34393.

Council of Science Editors:

Moore KM. Tatooine's Future: Dynamical Evolution of Planets Orbiting Two Stars. [Masters Thesis]. York University; 2018. Available from: http://hdl.handle.net/10315/34393


University of Arizona

24. Boroson, Todd Allan. CHEMICAL ABUNDANCES AND PHOTOMETRIC PARAMETERS IN THE BULGES OF SPIRAL GALAXIES .

Degree: 1980, University of Arizona

 The relation between central or mean metallicity and luminosity in elliptical galaxies is a well observed phenomenon. Theoretical explanations proposed for this relation include scenarios… (more)

Subjects/Keywords: Galaxies  – Spectra.; Galaxies  – Evolution.; Stars  – Evolution.

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APA (6th Edition):

Boroson, T. A. (1980). CHEMICAL ABUNDANCES AND PHOTOMETRIC PARAMETERS IN THE BULGES OF SPIRAL GALAXIES . (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/282503

Chicago Manual of Style (16th Edition):

Boroson, Todd Allan. “CHEMICAL ABUNDANCES AND PHOTOMETRIC PARAMETERS IN THE BULGES OF SPIRAL GALAXIES .” 1980. Doctoral Dissertation, University of Arizona. Accessed March 08, 2021. http://hdl.handle.net/10150/282503.

MLA Handbook (7th Edition):

Boroson, Todd Allan. “CHEMICAL ABUNDANCES AND PHOTOMETRIC PARAMETERS IN THE BULGES OF SPIRAL GALAXIES .” 1980. Web. 08 Mar 2021.

Vancouver:

Boroson TA. CHEMICAL ABUNDANCES AND PHOTOMETRIC PARAMETERS IN THE BULGES OF SPIRAL GALAXIES . [Internet] [Doctoral dissertation]. University of Arizona; 1980. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/10150/282503.

Council of Science Editors:

Boroson TA. CHEMICAL ABUNDANCES AND PHOTOMETRIC PARAMETERS IN THE BULGES OF SPIRAL GALAXIES . [Doctoral Dissertation]. University of Arizona; 1980. Available from: http://hdl.handle.net/10150/282503

25. Amard, Louis. Évolution de la rotation des étoiles jeunes de faible masse : Rotational evolution of young low-mass stars.

Degree: Docteur es, Physique, 2016, Montpellier; Observatoire de Genève (Suisse)

Le moment cinétique d’une étoile, comme sa masse ou sa composition chimique, est l’une de ses propriétés fondamentales, l’un de celles qui varient à cours… (more)

Subjects/Keywords: Evolution stellaire; Rotation; Magnétohydrodynamique; Etoiles jeunes; Stellar Evolution; Rotation; Young stars; Magnetohydrodynamics

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APA (6th Edition):

Amard, L. (2016). Évolution de la rotation des étoiles jeunes de faible masse : Rotational evolution of young low-mass stars. (Doctoral Dissertation). Montpellier; Observatoire de Genève (Suisse). Retrieved from http://www.theses.fr/2016MONTT258

Chicago Manual of Style (16th Edition):

Amard, Louis. “Évolution de la rotation des étoiles jeunes de faible masse : Rotational evolution of young low-mass stars.” 2016. Doctoral Dissertation, Montpellier; Observatoire de Genève (Suisse). Accessed March 08, 2021. http://www.theses.fr/2016MONTT258.

MLA Handbook (7th Edition):

Amard, Louis. “Évolution de la rotation des étoiles jeunes de faible masse : Rotational evolution of young low-mass stars.” 2016. Web. 08 Mar 2021.

Vancouver:

Amard L. Évolution de la rotation des étoiles jeunes de faible masse : Rotational evolution of young low-mass stars. [Internet] [Doctoral dissertation]. Montpellier; Observatoire de Genève (Suisse); 2016. [cited 2021 Mar 08]. Available from: http://www.theses.fr/2016MONTT258.

Council of Science Editors:

Amard L. Évolution de la rotation des étoiles jeunes de faible masse : Rotational evolution of young low-mass stars. [Doctoral Dissertation]. Montpellier; Observatoire de Genève (Suisse); 2016. Available from: http://www.theses.fr/2016MONTT258


Macquarie University

26. Douchin, Dimitri. Estimating the binary fraction of central stars of planetary nebulae.

Degree: 2015, Macquarie University

"A PhD thesis submitted to Macquarie University in cotutelle with Université de Montpellier 2 Department of Physics and Astronomy January 2015"

Abstract and summary also… (more)

Subjects/Keywords: Planetary nebulae; Double stars  – Evolution; stellar physics; astronomy; astrophysics; planetary nebula; binary star; stellar evolution

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APA (6th Edition):

Douchin, D. (2015). Estimating the binary fraction of central stars of planetary nebulae. (Doctoral Dissertation). Macquarie University. Retrieved from http://hdl.handle.net/1959.14/1068333

Chicago Manual of Style (16th Edition):

Douchin, Dimitri. “Estimating the binary fraction of central stars of planetary nebulae.” 2015. Doctoral Dissertation, Macquarie University. Accessed March 08, 2021. http://hdl.handle.net/1959.14/1068333.

MLA Handbook (7th Edition):

Douchin, Dimitri. “Estimating the binary fraction of central stars of planetary nebulae.” 2015. Web. 08 Mar 2021.

Vancouver:

Douchin D. Estimating the binary fraction of central stars of planetary nebulae. [Internet] [Doctoral dissertation]. Macquarie University; 2015. [cited 2021 Mar 08]. Available from: http://hdl.handle.net/1959.14/1068333.

Council of Science Editors:

Douchin D. Estimating the binary fraction of central stars of planetary nebulae. [Doctoral Dissertation]. Macquarie University; 2015. Available from: http://hdl.handle.net/1959.14/1068333


Rochester Institute of Technology

27. Freeman, Marcus J. Multiwavelength Imaging of Planetary Nebulae: Resolving & Disentangling Structure.

Degree: PhD, School of Physics and Astronomy (COS), 2015, Rochester Institute of Technology

  Planetary nebulae (PNe) represent the late stages of low-mass stellar evolution. The formation of the myriad of PNe morphologies involves processes that are present… (more)

Subjects/Keywords: Modeling; Planetary nebulae; Stars; Stellar evolution; X-rays

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APA (6th Edition):

Freeman, M. J. (2015). Multiwavelength Imaging of Planetary Nebulae: Resolving & Disentangling Structure. (Doctoral Dissertation). Rochester Institute of Technology. Retrieved from https://scholarworks.rit.edu/theses/8888

Chicago Manual of Style (16th Edition):

Freeman, Marcus J. “Multiwavelength Imaging of Planetary Nebulae: Resolving & Disentangling Structure.” 2015. Doctoral Dissertation, Rochester Institute of Technology. Accessed March 08, 2021. https://scholarworks.rit.edu/theses/8888.

MLA Handbook (7th Edition):

Freeman, Marcus J. “Multiwavelength Imaging of Planetary Nebulae: Resolving & Disentangling Structure.” 2015. Web. 08 Mar 2021.

Vancouver:

Freeman MJ. Multiwavelength Imaging of Planetary Nebulae: Resolving & Disentangling Structure. [Internet] [Doctoral dissertation]. Rochester Institute of Technology; 2015. [cited 2021 Mar 08]. Available from: https://scholarworks.rit.edu/theses/8888.

Council of Science Editors:

Freeman MJ. Multiwavelength Imaging of Planetary Nebulae: Resolving & Disentangling Structure. [Doctoral Dissertation]. Rochester Institute of Technology; 2015. Available from: https://scholarworks.rit.edu/theses/8888


Vilnius University

28. Stonkutė, Edita. Chemical composition of kinematically identified galactic stellar group.

Degree: PhD, Physics, 2013, Vilnius University

A number of stellar streams, moving and kinematic groups were identified in the Milky Way galaxy. Some of them are suspected to originate from accreted… (more)

Subjects/Keywords: Galaxy evolution; Formation; Stars; Abundance; Galaktikos evoliucija; Formavimasis; Žvaigždės; Gausos

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APA (6th Edition):

Stonkutė, E. (2013). Chemical composition of kinematically identified galactic stellar group. (Doctoral Dissertation). Vilnius University. Retrieved from http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2013~D_20130925_093107-33619 ;

Chicago Manual of Style (16th Edition):

Stonkutė, Edita. “Chemical composition of kinematically identified galactic stellar group.” 2013. Doctoral Dissertation, Vilnius University. Accessed March 08, 2021. http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2013~D_20130925_093107-33619 ;.

MLA Handbook (7th Edition):

Stonkutė, Edita. “Chemical composition of kinematically identified galactic stellar group.” 2013. Web. 08 Mar 2021.

Vancouver:

Stonkutė E. Chemical composition of kinematically identified galactic stellar group. [Internet] [Doctoral dissertation]. Vilnius University; 2013. [cited 2021 Mar 08]. Available from: http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2013~D_20130925_093107-33619 ;.

Council of Science Editors:

Stonkutė E. Chemical composition of kinematically identified galactic stellar group. [Doctoral Dissertation]. Vilnius University; 2013. Available from: http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2013~D_20130925_093107-33619 ;


Vilnius University

29. Stonkutė, Edita. Cheminė kinematiškai identifikuotos Galaktikos žvaigždžių grupės sudėtis.

Degree: Dissertation, Physics, 2013, Vilnius University

Paukščių Tako galaktikoje yra identifikuota žvaigždžių srautų, judančių bei kinematinių grupių, kurių kilmė siejama su įkritusiomis galaktikomis. Aktualu ištirti, ar yra tokių senųjų substruktūrų pėdsakų… (more)

Subjects/Keywords: Galatikos evoliucija; Formavimasis; Žvaigždės; Gausos; Galaxy evolution; Formation; Stars; Abundance

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APA (6th Edition):

Stonkutė, E. (2013). Cheminė kinematiškai identifikuotos Galaktikos žvaigždžių grupės sudėtis. (Doctoral Dissertation). Vilnius University. Retrieved from http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2013~D_20130925_093256-69980 ;

Chicago Manual of Style (16th Edition):

Stonkutė, Edita. “Cheminė kinematiškai identifikuotos Galaktikos žvaigždžių grupės sudėtis.” 2013. Doctoral Dissertation, Vilnius University. Accessed March 08, 2021. http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2013~D_20130925_093256-69980 ;.

MLA Handbook (7th Edition):

Stonkutė, Edita. “Cheminė kinematiškai identifikuotos Galaktikos žvaigždžių grupės sudėtis.” 2013. Web. 08 Mar 2021.

Vancouver:

Stonkutė E. Cheminė kinematiškai identifikuotos Galaktikos žvaigždžių grupės sudėtis. [Internet] [Doctoral dissertation]. Vilnius University; 2013. [cited 2021 Mar 08]. Available from: http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2013~D_20130925_093256-69980 ;.

Council of Science Editors:

Stonkutė E. Cheminė kinematiškai identifikuotos Galaktikos žvaigždžių grupės sudėtis. [Doctoral Dissertation]. Vilnius University; 2013. Available from: http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2013~D_20130925_093256-69980 ;

30. Potter, Adrian Thomas. Rotation and magnetism in massive stars.

Degree: PhD, 2012, University of Cambridge

 Rotation has a number of important effects on the evolution of stars. Apart from structural changes because of the centrifugal force, turbulent mixing and meridional… (more)

Subjects/Keywords: Stars; Astronomy; Rotation; Magnetic; Chemically peculiar; Evolution; Stellar

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

APA (6th Edition):

Potter, A. T. (2012). Rotation and magnetism in massive stars. (Doctoral Dissertation). University of Cambridge. Retrieved from http://www.dspace.cam.ac.uk/handle/1810/243617https://www.repository.cam.ac.uk/bitstream/1810/243617/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/3/license_url ; https://www.repository.cam.ac.uk/bitstream/1810/243617/4/license_text ; https://www.repository.cam.ac.uk/bitstream/1810/243617/5/license_rdf ; https://www.repository.cam.ac.uk/bitstream/1810/243617/9/potterThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/7/potterThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/10/potterThesis.pdf.jpg

Chicago Manual of Style (16th Edition):

Potter, Adrian Thomas. “Rotation and magnetism in massive stars.” 2012. Doctoral Dissertation, University of Cambridge. Accessed March 08, 2021. http://www.dspace.cam.ac.uk/handle/1810/243617https://www.repository.cam.ac.uk/bitstream/1810/243617/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/3/license_url ; https://www.repository.cam.ac.uk/bitstream/1810/243617/4/license_text ; https://www.repository.cam.ac.uk/bitstream/1810/243617/5/license_rdf ; https://www.repository.cam.ac.uk/bitstream/1810/243617/9/potterThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/7/potterThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/10/potterThesis.pdf.jpg.

MLA Handbook (7th Edition):

Potter, Adrian Thomas. “Rotation and magnetism in massive stars.” 2012. Web. 08 Mar 2021.

Vancouver:

Potter AT. Rotation and magnetism in massive stars. [Internet] [Doctoral dissertation]. University of Cambridge; 2012. [cited 2021 Mar 08]. Available from: http://www.dspace.cam.ac.uk/handle/1810/243617https://www.repository.cam.ac.uk/bitstream/1810/243617/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/3/license_url ; https://www.repository.cam.ac.uk/bitstream/1810/243617/4/license_text ; https://www.repository.cam.ac.uk/bitstream/1810/243617/5/license_rdf ; https://www.repository.cam.ac.uk/bitstream/1810/243617/9/potterThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/7/potterThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/10/potterThesis.pdf.jpg.

Council of Science Editors:

Potter AT. Rotation and magnetism in massive stars. [Doctoral Dissertation]. University of Cambridge; 2012. Available from: http://www.dspace.cam.ac.uk/handle/1810/243617https://www.repository.cam.ac.uk/bitstream/1810/243617/2/license.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/3/license_url ; https://www.repository.cam.ac.uk/bitstream/1810/243617/4/license_text ; https://www.repository.cam.ac.uk/bitstream/1810/243617/5/license_rdf ; https://www.repository.cam.ac.uk/bitstream/1810/243617/9/potterThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/7/potterThesis.pdf.txt ; https://www.repository.cam.ac.uk/bitstream/1810/243617/10/potterThesis.pdf.jpg

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