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You searched for subject:(Stellar rotation). Showing records 1 – 29 of 29 total matches.

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Clemson University

1. Tannous, Jaad Antoun. The Effect of Rotation on Stellar Structure and Evolution.

Degree: MS, Physics and Astronomy, 2020, Clemson University

  In this thesis, we investigate the eects of rotation on the evolution of stars in the mass range of 2-15 M assuming solar-like initial… (more)

Subjects/Keywords: Rotation; s-process; Stellar Evolution; Stellar Structure

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APA (6th Edition):

Tannous, J. A. (2020). The Effect of Rotation on Stellar Structure and Evolution. (Masters Thesis). Clemson University. Retrieved from https://tigerprints.clemson.edu/all_theses/3267

Chicago Manual of Style (16th Edition):

Tannous, Jaad Antoun. “The Effect of Rotation on Stellar Structure and Evolution.” 2020. Masters Thesis, Clemson University. Accessed March 05, 2021. https://tigerprints.clemson.edu/all_theses/3267.

MLA Handbook (7th Edition):

Tannous, Jaad Antoun. “The Effect of Rotation on Stellar Structure and Evolution.” 2020. Web. 05 Mar 2021.

Vancouver:

Tannous JA. The Effect of Rotation on Stellar Structure and Evolution. [Internet] [Masters thesis]. Clemson University; 2020. [cited 2021 Mar 05]. Available from: https://tigerprints.clemson.edu/all_theses/3267.

Council of Science Editors:

Tannous JA. The Effect of Rotation on Stellar Structure and Evolution. [Masters Thesis]. Clemson University; 2020. Available from: https://tigerprints.clemson.edu/all_theses/3267


University of Sydney

2. Maestro, Vicente. Interferometric observations of hot stars .

Degree: 2014, University of Sydney

 Accurate determination of fundamental stellar properties is crucial in understanding and testing models of stellar structure and evolution. To date, most stars with independent determinations… (more)

Subjects/Keywords: Optical Interferometry; Stellar Astrophysics; Stellar rotation

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APA (6th Edition):

Maestro, V. (2014). Interferometric observations of hot stars . (Thesis). University of Sydney. Retrieved from http://hdl.handle.net/2123/11671

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):

Maestro, Vicente. “Interferometric observations of hot stars .” 2014. Thesis, University of Sydney. Accessed March 05, 2021. http://hdl.handle.net/2123/11671.

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

MLA Handbook (7th Edition):

Maestro, Vicente. “Interferometric observations of hot stars .” 2014. Web. 05 Mar 2021.

Vancouver:

Maestro V. Interferometric observations of hot stars . [Internet] [Thesis]. University of Sydney; 2014. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/2123/11671.

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

Council of Science Editors:

Maestro V. Interferometric observations of hot stars . [Thesis]. University of Sydney; 2014. Available from: http://hdl.handle.net/2123/11671

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


University of Oxford

3. McQuillan, Amy. Stellar variability and rotation in Kepler planetary transit search data.

Degree: PhD, 2013, University of Oxford

 The recent space-based exoplanet transit searches, CoRoT and Kepler, have revolutionised the field of stellar variability. In this thesis I exploit the public Kepler data… (more)

Subjects/Keywords: 523.8; Astrophysics; stellar physics; stellar rotation; stellar variability; systematics removal

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APA (6th Edition):

McQuillan, A. (2013). Stellar variability and rotation in Kepler planetary transit search data. (Doctoral Dissertation). University of Oxford. Retrieved from http://ora.ox.ac.uk/objects/uuid:802a873d-650f-4f0b-b814-f8397b2798e2 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.618438

Chicago Manual of Style (16th Edition):

McQuillan, Amy. “Stellar variability and rotation in Kepler planetary transit search data.” 2013. Doctoral Dissertation, University of Oxford. Accessed March 05, 2021. http://ora.ox.ac.uk/objects/uuid:802a873d-650f-4f0b-b814-f8397b2798e2 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.618438.

MLA Handbook (7th Edition):

McQuillan, Amy. “Stellar variability and rotation in Kepler planetary transit search data.” 2013. Web. 05 Mar 2021.

Vancouver:

McQuillan A. Stellar variability and rotation in Kepler planetary transit search data. [Internet] [Doctoral dissertation]. University of Oxford; 2013. [cited 2021 Mar 05]. Available from: http://ora.ox.ac.uk/objects/uuid:802a873d-650f-4f0b-b814-f8397b2798e2 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.618438.

Council of Science Editors:

McQuillan A. Stellar variability and rotation in Kepler planetary transit search data. [Doctoral Dissertation]. University of Oxford; 2013. Available from: http://ora.ox.ac.uk/objects/uuid:802a873d-650f-4f0b-b814-f8397b2798e2 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.618438

4. Mirouh, Giovanni Marcello. Rôle de la rotation différentielle sur le spectre basse fréquence des étoiles en rotation rapide : Role of differential rotation on low-frequency oscillation spectra of fast-rotating stars.

Degree: Docteur es, Astrophysique, 2016, Université Toulouse III – Paul Sabatier

Les étoiles massives sont les principaux contributeurs à l'enrichissement du milieu interstellaire. Ce sont généralement des rotateurs rapides, dotés d'une enveloppe radiative dans laquelle l'interaction… (more)

Subjects/Keywords: Etoiles; Oscillations stellaires; Etoiles en rotation; Rotation différentielle; Astérosismologie; Instabilités; Stars; Stellar pulsations; Stellar rotation; Differential rotation; Asteroseismology; Baroclinic instabilities

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APA (6th Edition):

Mirouh, G. M. (2016). Rôle de la rotation différentielle sur le spectre basse fréquence des étoiles en rotation rapide : Role of differential rotation on low-frequency oscillation spectra of fast-rotating stars. (Doctoral Dissertation). Université Toulouse III – Paul Sabatier. Retrieved from http://www.theses.fr/2016TOU30374

Chicago Manual of Style (16th Edition):

Mirouh, Giovanni Marcello. “Rôle de la rotation différentielle sur le spectre basse fréquence des étoiles en rotation rapide : Role of differential rotation on low-frequency oscillation spectra of fast-rotating stars.” 2016. Doctoral Dissertation, Université Toulouse III – Paul Sabatier. Accessed March 05, 2021. http://www.theses.fr/2016TOU30374.

MLA Handbook (7th Edition):

Mirouh, Giovanni Marcello. “Rôle de la rotation différentielle sur le spectre basse fréquence des étoiles en rotation rapide : Role of differential rotation on low-frequency oscillation spectra of fast-rotating stars.” 2016. Web. 05 Mar 2021.

Vancouver:

Mirouh GM. Rôle de la rotation différentielle sur le spectre basse fréquence des étoiles en rotation rapide : Role of differential rotation on low-frequency oscillation spectra of fast-rotating stars. [Internet] [Doctoral dissertation]. Université Toulouse III – Paul Sabatier; 2016. [cited 2021 Mar 05]. Available from: http://www.theses.fr/2016TOU30374.

Council of Science Editors:

Mirouh GM. Rôle de la rotation différentielle sur le spectre basse fréquence des étoiles en rotation rapide : Role of differential rotation on low-frequency oscillation spectra of fast-rotating stars. [Doctoral Dissertation]. Université Toulouse III – Paul Sabatier; 2016. Available from: http://www.theses.fr/2016TOU30374


The Ohio State University

5. Tayar, Jamie Nicole. Rotation in Red Giants.

Degree: PhD, Astronomy, 2018, The Ohio State University

 Real stars rotate, and rotation can have profound consequences for stellar structure and evolution. Despite this, rotation is frequently ignored in evolved stars, or treated… (more)

Subjects/Keywords: Astronomy; stars; stellar evolution; stellar rotation; red giants

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APA (6th Edition):

Tayar, J. N. (2018). Rotation in Red Giants. (Doctoral Dissertation). The Ohio State University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=osu1531927526281553

Chicago Manual of Style (16th Edition):

Tayar, Jamie Nicole. “Rotation in Red Giants.” 2018. Doctoral Dissertation, The Ohio State University. Accessed March 05, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=osu1531927526281553.

MLA Handbook (7th Edition):

Tayar, Jamie Nicole. “Rotation in Red Giants.” 2018. Web. 05 Mar 2021.

Vancouver:

Tayar JN. Rotation in Red Giants. [Internet] [Doctoral dissertation]. The Ohio State University; 2018. [cited 2021 Mar 05]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1531927526281553.

Council of Science Editors:

Tayar JN. Rotation in Red Giants. [Doctoral Dissertation]. The Ohio State University; 2018. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1531927526281553

6. 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 05, 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. 05 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 05]. 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

7. Jendreieck, Andressa Maria. Sismologia e Rotação ao Longo da Sequência Principal.

Degree: Mestrado, Astronomia, 2011, University of São Paulo

A sismologia estelar oferece uma oportunidade única de sondar as propriedades internas das estrelas através do estudo de oscilações estelares. Essas oscilações são dependentes diretamente… (more)

Subjects/Keywords: Asteroseismology; modelos oscilatórios.; Oscillatory Models.; rotação estelar; Sismologia estelar; Stellar Rotation

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APA (6th Edition):

Jendreieck, A. M. (2011). Sismologia e Rotação ao Longo da Sequência Principal. (Masters Thesis). University of São Paulo. Retrieved from http://www.teses.usp.br/teses/disponiveis/14/14131/tde-27042011-164107/ ;

Chicago Manual of Style (16th Edition):

Jendreieck, Andressa Maria. “Sismologia e Rotação ao Longo da Sequência Principal.” 2011. Masters Thesis, University of São Paulo. Accessed March 05, 2021. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-27042011-164107/ ;.

MLA Handbook (7th Edition):

Jendreieck, Andressa Maria. “Sismologia e Rotação ao Longo da Sequência Principal.” 2011. Web. 05 Mar 2021.

Vancouver:

Jendreieck AM. Sismologia e Rotação ao Longo da Sequência Principal. [Internet] [Masters thesis]. University of São Paulo; 2011. [cited 2021 Mar 05]. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-27042011-164107/ ;.

Council of Science Editors:

Jendreieck AM. Sismologia e Rotação ao Longo da Sequência Principal. [Masters Thesis]. University of São Paulo; 2011. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-27042011-164107/ ;

8. 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 (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 05, 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. 05 Mar 2021.

Vancouver:

Potter AT. Rotation and magnetism in massive stars. [Internet] [Doctoral dissertation]. University of Cambridge; 2012. [cited 2021 Mar 05]. 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

9. Zayer, Imad. Searching for Rotational and Activity Signals in M Dwarf Stars.

Degree: 2017, University of Hertfordshire

 We search for signals coming from M dwarf stars through variations caused by stellar surface activity. The aims of this work are to find the… (more)

Subjects/Keywords: exoplanet; rotation periods; M dwarfs; stellar activity; aliases; periodogram; ASAS photometric

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APA (6th Edition):

Zayer, I. (2017). Searching for Rotational and Activity Signals in M Dwarf Stars. (Masters Thesis). University of Hertfordshire. Retrieved from http://hdl.handle.net/2299/18729

Chicago Manual of Style (16th Edition):

Zayer, Imad. “Searching for Rotational and Activity Signals in M Dwarf Stars.” 2017. Masters Thesis, University of Hertfordshire. Accessed March 05, 2021. http://hdl.handle.net/2299/18729.

MLA Handbook (7th Edition):

Zayer, Imad. “Searching for Rotational and Activity Signals in M Dwarf Stars.” 2017. Web. 05 Mar 2021.

Vancouver:

Zayer I. Searching for Rotational and Activity Signals in M Dwarf Stars. [Internet] [Masters thesis]. University of Hertfordshire; 2017. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/2299/18729.

Council of Science Editors:

Zayer I. Searching for Rotational and Activity Signals in M Dwarf Stars. [Masters Thesis]. University of Hertfordshire; 2017. Available from: http://hdl.handle.net/2299/18729


University of Cambridge

10. 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: 520; Stars; Astronomy; Rotation; Magnetic; Chemically peculiar; Evolution; Stellar

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APA (6th Edition):

Potter, A. T. (2012). Rotation and magnetism in massive stars. (Doctoral Dissertation). University of Cambridge. Retrieved from https://doi.org/10.17863/CAM.15999 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.556241

Chicago Manual of Style (16th Edition):

Potter, Adrian Thomas. “Rotation and magnetism in massive stars.” 2012. Doctoral Dissertation, University of Cambridge. Accessed March 05, 2021. https://doi.org/10.17863/CAM.15999 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.556241.

MLA Handbook (7th Edition):

Potter, Adrian Thomas. “Rotation and magnetism in massive stars.” 2012. Web. 05 Mar 2021.

Vancouver:

Potter AT. Rotation and magnetism in massive stars. [Internet] [Doctoral dissertation]. University of Cambridge; 2012. [cited 2021 Mar 05]. Available from: https://doi.org/10.17863/CAM.15999 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.556241.

Council of Science Editors:

Potter AT. Rotation and magnetism in massive stars. [Doctoral Dissertation]. University of Cambridge; 2012. Available from: https://doi.org/10.17863/CAM.15999 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.556241


University of Sydney

11. Li, Gang. Asteroseismology of gamma Doradus stars with Kepler .

Degree: 2020, University of Sydney

Stellar physics is a vital part of modern astronomy. To better understand stars, we must understand not only the stellar surface, but also the stellar(more)

Subjects/Keywords: Asteroseismology; stellar rotation; gamma Doradus stars; eclipsing binaries

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APA (6th Edition):

Li, G. (2020). Asteroseismology of gamma Doradus stars with Kepler . (Thesis). University of Sydney. Retrieved from http://hdl.handle.net/2123/23393

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):

Li, Gang. “Asteroseismology of gamma Doradus stars with Kepler .” 2020. Thesis, University of Sydney. Accessed March 05, 2021. http://hdl.handle.net/2123/23393.

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

MLA Handbook (7th Edition):

Li, Gang. “Asteroseismology of gamma Doradus stars with Kepler .” 2020. Web. 05 Mar 2021.

Vancouver:

Li G. Asteroseismology of gamma Doradus stars with Kepler . [Internet] [Thesis]. University of Sydney; 2020. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/2123/23393.

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

Council of Science Editors:

Li G. Asteroseismology of gamma Doradus stars with Kepler . [Thesis]. University of Sydney; 2020. Available from: http://hdl.handle.net/2123/23393

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

12. Taiza Alissul Sauer do Carmo. Espectroscopia de Estrelas Be nos aglomerados NGC 4755 e NGC 6530.

Degree: 2008, UNIVERSIDADE ESTADUAL DE PONTA GROSSA

Uma das principais teorias para explicar o fenômeno Be é que são estrelas quentes com velocidade de rotação próxima da velocidade crítica, ejetando matéria formando… (more)

Subjects/Keywords: espectroscopia estelar; estrelas Be; linhas de Balmer; rotação estelar; stellar spectroscopy; Be stars; Balmer lines; stellar rotation; FISICA

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APA (6th Edition):

Carmo, T. A. S. d. (2008). Espectroscopia de Estrelas Be nos aglomerados NGC 4755 e NGC 6530. (Thesis). UNIVERSIDADE ESTADUAL DE PONTA GROSSA. Retrieved from http://www.bicen-tede.uepg.br/tde_busca/arquivo.php?codArquivo=174

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):

Carmo, Taiza Alissul Sauer do. “Espectroscopia de Estrelas Be nos aglomerados NGC 4755 e NGC 6530.” 2008. Thesis, UNIVERSIDADE ESTADUAL DE PONTA GROSSA. Accessed March 05, 2021. http://www.bicen-tede.uepg.br/tde_busca/arquivo.php?codArquivo=174.

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

MLA Handbook (7th Edition):

Carmo, Taiza Alissul Sauer do. “Espectroscopia de Estrelas Be nos aglomerados NGC 4755 e NGC 6530.” 2008. Web. 05 Mar 2021.

Vancouver:

Carmo TASd. Espectroscopia de Estrelas Be nos aglomerados NGC 4755 e NGC 6530. [Internet] [Thesis]. UNIVERSIDADE ESTADUAL DE PONTA GROSSA; 2008. [cited 2021 Mar 05]. Available from: http://www.bicen-tede.uepg.br/tde_busca/arquivo.php?codArquivo=174.

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

Council of Science Editors:

Carmo TASd. Espectroscopia de Estrelas Be nos aglomerados NGC 4755 e NGC 6530. [Thesis]. UNIVERSIDADE ESTADUAL DE PONTA GROSSA; 2008. Available from: http://www.bicen-tede.uepg.br/tde_busca/arquivo.php?codArquivo=174

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

13. Notsu, Yuta. Observational studies on solar-type superflare stars .

Degree: 2019, Kyoto University

Subjects/Keywords: stellar flare; superflare; starspot; solar-type stars; stellar rotation

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APA (6th Edition):

Notsu, Y. (2019). Observational studies on solar-type superflare stars . (Thesis). Kyoto University. Retrieved from http://hdl.handle.net/2433/242613

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):

Notsu, Yuta. “Observational studies on solar-type superflare stars .” 2019. Thesis, Kyoto University. Accessed March 05, 2021. http://hdl.handle.net/2433/242613.

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

MLA Handbook (7th Edition):

Notsu, Yuta. “Observational studies on solar-type superflare stars .” 2019. Web. 05 Mar 2021.

Vancouver:

Notsu Y. Observational studies on solar-type superflare stars . [Internet] [Thesis]. Kyoto University; 2019. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/2433/242613.

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

Council of Science Editors:

Notsu Y. Observational studies on solar-type superflare stars . [Thesis]. Kyoto University; 2019. Available from: http://hdl.handle.net/2433/242613

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

14. van Saders, Jennifer Lynn. Using Modern Stellar Observables to Constrain Stellar Parameters and the Physics of the Stellar Interior.

Degree: PhD, Astronomy, 2014, The Ohio State University

 The current state and future evolution of a star is, in principle, specified by a only a few physical quantities: the mass, age, hydrogen, helium,… (more)

Subjects/Keywords: Astrophysics; Astronomy; stars; stellar evolution; stellar rotation; asteroseismology; stellar structure

…Star; Old Star, Young Star: Subgiant Rotation as a Population and Stellar Physics Diagnostic… …Asteroseismology . . . . . . . . . . . . . . . . . 5 1.4 Modern Observables: Stellar Rotation… …of Model Predictions with Observations . . . . . . 98 Stellar Rotation as a Tool… …inertia for a range of stellar masses. . . . . . . . . . . 122 4.2 Theoretical rotation… …constrain stellar parameters and interiors. 1.4. Modern Observables: Stellar Rotation All stars… 

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APA (6th Edition):

van Saders, J. L. (2014). Using Modern Stellar Observables to Constrain Stellar Parameters and the Physics of the Stellar Interior. (Doctoral Dissertation). The Ohio State University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=osu1404130939

Chicago Manual of Style (16th Edition):

van Saders, Jennifer Lynn. “Using Modern Stellar Observables to Constrain Stellar Parameters and the Physics of the Stellar Interior.” 2014. Doctoral Dissertation, The Ohio State University. Accessed March 05, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=osu1404130939.

MLA Handbook (7th Edition):

van Saders, Jennifer Lynn. “Using Modern Stellar Observables to Constrain Stellar Parameters and the Physics of the Stellar Interior.” 2014. Web. 05 Mar 2021.

Vancouver:

van Saders JL. Using Modern Stellar Observables to Constrain Stellar Parameters and the Physics of the Stellar Interior. [Internet] [Doctoral dissertation]. The Ohio State University; 2014. [cited 2021 Mar 05]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1404130939.

Council of Science Editors:

van Saders JL. Using Modern Stellar Observables to Constrain Stellar Parameters and the Physics of the Stellar Interior. [Doctoral Dissertation]. The Ohio State University; 2014. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1404130939

15. Junqueira, Thiago Correr. Determinação da curva de rotação galática e estudo do mínimo próximo a R0.

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

A curva de rotação da Galáxia apresenta uma anomalia perto do raio da órbita solar R0, caracterizada pela presença de um mínimo. Existem trabalhos que,… (more)

Subjects/Keywords: Cinemática Estelar; Curva de Rotação; Estrutura da Galáxia; galactic constant measurements.; Rotation curve; stellar kinematics

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APA (6th Edition):

Junqueira, T. C. (2009). Determinação da curva de rotação galática e estudo do mínimo próximo a R0. (Masters Thesis). University of São Paulo. Retrieved from http://www.teses.usp.br/teses/disponiveis/14/14131/tde-10092009-125714/ ;

Chicago Manual of Style (16th Edition):

Junqueira, Thiago Correr. “Determinação da curva de rotação galática e estudo do mínimo próximo a R0.” 2009. Masters Thesis, University of São Paulo. Accessed March 05, 2021. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-10092009-125714/ ;.

MLA Handbook (7th Edition):

Junqueira, Thiago Correr. “Determinação da curva de rotação galática e estudo do mínimo próximo a R0.” 2009. Web. 05 Mar 2021.

Vancouver:

Junqueira TC. Determinação da curva de rotação galática e estudo do mínimo próximo a R0. [Internet] [Masters thesis]. University of São Paulo; 2009. [cited 2021 Mar 05]. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-10092009-125714/ ;.

Council of Science Editors:

Junqueira TC. Determinação da curva de rotação galática e estudo do mínimo próximo a R0. [Masters Thesis]. University of São Paulo; 2009. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-10092009-125714/ ;


Universidade do Rio Grande do Norte

16. Nascimento, Sanzia Alves do. Propriedades físicas de planetas extrasolares .

Degree: 2008, Universidade do Rio Grande do Norte

ROTATION is one the most important aspects to be observed in stellar astrophysics. Here we investigate that particularly in stars with planets. This physical parameter… (more)

Subjects/Keywords: Rotação estelar; Exoplanetas; Momento angular; Estrelas hospedeiras; Parâmetros físicos; Stellar rotation; Exoplanets; Angular momentum; Stars with planets; Physical parameter

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APA (6th Edition):

Nascimento, S. A. d. (2008). Propriedades físicas de planetas extrasolares . (Thesis). Universidade do Rio Grande do Norte. Retrieved from http://repositorio.ufrn.br/handle/123456789/18579

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):

Nascimento, Sanzia Alves do. “Propriedades físicas de planetas extrasolares .” 2008. Thesis, Universidade do Rio Grande do Norte. Accessed March 05, 2021. http://repositorio.ufrn.br/handle/123456789/18579.

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

MLA Handbook (7th Edition):

Nascimento, Sanzia Alves do. “Propriedades físicas de planetas extrasolares .” 2008. Web. 05 Mar 2021.

Vancouver:

Nascimento SAd. Propriedades físicas de planetas extrasolares . [Internet] [Thesis]. Universidade do Rio Grande do Norte; 2008. [cited 2021 Mar 05]. Available from: http://repositorio.ufrn.br/handle/123456789/18579.

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

Council of Science Editors:

Nascimento SAd. Propriedades físicas de planetas extrasolares . [Thesis]. Universidade do Rio Grande do Norte; 2008. Available from: http://repositorio.ufrn.br/handle/123456789/18579

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

17. Sanzia Alves do Nascimento. Propriedades físicas de planetas extrasolares.

Degree: 2008, Universidade Federal do Rio Grande do Norte

ROTAÇÃO é um dos importantes aspectos a ser observado na astrofísica estelar. Por isto, neste trabalho, investigamos este parâmetro no estudo das estrelas hospedeiras de… (more)

Subjects/Keywords: Rotação estelar; Exoplanetas; Momento angular; Estrelas hospedeiras; Parâmetros físicos; ASTROFISICA ESTELAR; Stellar rotation; Exoplanets; Angular momentum; Stars with planets; Physical parameter

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APA (6th Edition):

Nascimento, S. A. d. (2008). Propriedades físicas de planetas extrasolares. (Thesis). Universidade Federal do Rio Grande do Norte. Retrieved from http://bdtd.bczm.ufrn.br/tedesimplificado//tde_busca/arquivo.php?codArquivo=2027

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):

Nascimento, Sanzia Alves do. “Propriedades físicas de planetas extrasolares.” 2008. Thesis, Universidade Federal do Rio Grande do Norte. Accessed March 05, 2021. http://bdtd.bczm.ufrn.br/tedesimplificado//tde_busca/arquivo.php?codArquivo=2027.

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

MLA Handbook (7th Edition):

Nascimento, Sanzia Alves do. “Propriedades físicas de planetas extrasolares.” 2008. Web. 05 Mar 2021.

Vancouver:

Nascimento SAd. Propriedades físicas de planetas extrasolares. [Internet] [Thesis]. Universidade Federal do Rio Grande do Norte; 2008. [cited 2021 Mar 05]. Available from: http://bdtd.bczm.ufrn.br/tedesimplificado//tde_busca/arquivo.php?codArquivo=2027.

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

Council of Science Editors:

Nascimento SAd. Propriedades físicas de planetas extrasolares. [Thesis]. Universidade Federal do Rio Grande do Norte; 2008. Available from: http://bdtd.bczm.ufrn.br/tedesimplificado//tde_busca/arquivo.php?codArquivo=2027

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


Universidade do Rio Grande do Norte

18. Nascimento, Sanzia Alves do. Propriedades físicas de planetas extrasolares .

Degree: 2008, Universidade do Rio Grande do Norte

ROTATION is one the most important aspects to be observed in stellar astrophysics. Here we investigate that particularly in stars with planets. This physical parameter… (more)

Subjects/Keywords: Rotação estelar; Exoplanetas; Momento angular; Estrelas hospedeiras; Parâmetros físicos; Stellar rotation; Exoplanets; Angular momentum; Stars with planets; Physical parameter

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

APA (6th Edition):

Nascimento, S. A. d. (2008). Propriedades físicas de planetas extrasolares . (Masters Thesis). Universidade do Rio Grande do Norte. Retrieved from http://repositorio.ufrn.br/handle/123456789/18579

Chicago Manual of Style (16th Edition):

Nascimento, Sanzia Alves do. “Propriedades físicas de planetas extrasolares .” 2008. Masters Thesis, Universidade do Rio Grande do Norte. Accessed March 05, 2021. http://repositorio.ufrn.br/handle/123456789/18579.

MLA Handbook (7th Edition):

Nascimento, Sanzia Alves do. “Propriedades físicas de planetas extrasolares .” 2008. Web. 05 Mar 2021.

Vancouver:

Nascimento SAd. Propriedades físicas de planetas extrasolares . [Internet] [Masters thesis]. Universidade do Rio Grande do Norte; 2008. [cited 2021 Mar 05]. Available from: http://repositorio.ufrn.br/handle/123456789/18579.

Council of Science Editors:

Nascimento SAd. Propriedades físicas de planetas extrasolares . [Masters Thesis]. Universidade do Rio Grande do Norte; 2008. Available from: http://repositorio.ufrn.br/handle/123456789/18579


University of Exeter

19. Finley, A. Constraining the angular momentum-loss rates of the Sun and other Sun-like stars.

Degree: PhD, 2020, University of Exeter

Stellar rotation, convection, and magnetism are intricately linked in low-mass stars like the Sun. In their outer convective envelopes, the interplay of rotation and convection… (more)

Subjects/Keywords: solar wind; stellar winds; astrophysics; magnetohydrodynamics; numerical simulation; rotation period evolution; low-mass stars; sun-like stars

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APA (6th Edition):

Finley, A. (2020). Constraining the angular momentum-loss rates of the Sun and other Sun-like stars. (Doctoral Dissertation). University of Exeter. Retrieved from http://hdl.handle.net/10871/121115

Chicago Manual of Style (16th Edition):

Finley, A. “Constraining the angular momentum-loss rates of the Sun and other Sun-like stars.” 2020. Doctoral Dissertation, University of Exeter. Accessed March 05, 2021. http://hdl.handle.net/10871/121115.

MLA Handbook (7th Edition):

Finley, A. “Constraining the angular momentum-loss rates of the Sun and other Sun-like stars.” 2020. Web. 05 Mar 2021.

Vancouver:

Finley A. Constraining the angular momentum-loss rates of the Sun and other Sun-like stars. [Internet] [Doctoral dissertation]. University of Exeter; 2020. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/10871/121115.

Council of Science Editors:

Finley A. Constraining the angular momentum-loss rates of the Sun and other Sun-like stars. [Doctoral Dissertation]. University of Exeter; 2020. Available from: http://hdl.handle.net/10871/121115

20. Gehan, Charlotte. Évolution de la rotation du cœur des étoiles sur la branche des géantes rouges : des mesures à grande échelle vers une caractérisation du transport de moment cinétique : Evolution of the core rotation of red giant branch stars : from large-scale measurements towards a characterisation of the angular momentum transport.

Degree: Docteur es, Astronomie et Astrophysique, 2018, Paris Sciences et Lettres

L’astérosismologie consiste à sonder les intérieurs stellaires en détectant les ondes sismiques qui s’y propagent. Les géantes rouges, des étoiles évoluées peu massives dont l’hydrogène… (more)

Subjects/Keywords: Physique stellaire; Astérosismologie; Géantes rouges; Rotation interne; Traitement de données; Modélisation; Stellar physics; Asteroseismology; Red giants; Internal rotation; Data analysis; Modelling; 520

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APA (6th Edition):

Gehan, C. (2018). Évolution de la rotation du cœur des étoiles sur la branche des géantes rouges : des mesures à grande échelle vers une caractérisation du transport de moment cinétique : Evolution of the core rotation of red giant branch stars : from large-scale measurements towards a characterisation of the angular momentum transport. (Doctoral Dissertation). Paris Sciences et Lettres. Retrieved from http://www.theses.fr/2018PSLEO021

Chicago Manual of Style (16th Edition):

Gehan, Charlotte. “Évolution de la rotation du cœur des étoiles sur la branche des géantes rouges : des mesures à grande échelle vers une caractérisation du transport de moment cinétique : Evolution of the core rotation of red giant branch stars : from large-scale measurements towards a characterisation of the angular momentum transport.” 2018. Doctoral Dissertation, Paris Sciences et Lettres. Accessed March 05, 2021. http://www.theses.fr/2018PSLEO021.

MLA Handbook (7th Edition):

Gehan, Charlotte. “Évolution de la rotation du cœur des étoiles sur la branche des géantes rouges : des mesures à grande échelle vers une caractérisation du transport de moment cinétique : Evolution of the core rotation of red giant branch stars : from large-scale measurements towards a characterisation of the angular momentum transport.” 2018. Web. 05 Mar 2021.

Vancouver:

Gehan C. Évolution de la rotation du cœur des étoiles sur la branche des géantes rouges : des mesures à grande échelle vers une caractérisation du transport de moment cinétique : Evolution of the core rotation of red giant branch stars : from large-scale measurements towards a characterisation of the angular momentum transport. [Internet] [Doctoral dissertation]. Paris Sciences et Lettres; 2018. [cited 2021 Mar 05]. Available from: http://www.theses.fr/2018PSLEO021.

Council of Science Editors:

Gehan C. Évolution de la rotation du cœur des étoiles sur la branche des géantes rouges : des mesures à grande échelle vers une caractérisation du transport de moment cinétique : Evolution of the core rotation of red giant branch stars : from large-scale measurements towards a characterisation of the angular momentum transport. [Doctoral Dissertation]. Paris Sciences et Lettres; 2018. Available from: http://www.theses.fr/2018PSLEO021


University of Florida

21. Hoffmann, Sara Witherow. Variations of the H and K emission lines of singly ionized calcium in the eclipsing binary star system AR Lacertae.

Degree: 1983, University of Florida

Subjects/Keywords: Eclipses; Emission spectra; Latitude; Light curves; Spectroscopy; Starspots; Stellar evolution; Stellar rotation; Stellar spectra; Wavelengths; Astronomical spectroscopy; Eclipsing binaries  – Spectra

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APA (6th Edition):

Hoffmann, S. W. (1983). Variations of the H and K emission lines of singly ionized calcium in the eclipsing binary star system AR Lacertae. (Thesis). University of Florida. Retrieved from https://ufdc.ufl.edu/AA00003837

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):

Hoffmann, Sara Witherow. “Variations of the H and K emission lines of singly ionized calcium in the eclipsing binary star system AR Lacertae.” 1983. Thesis, University of Florida. Accessed March 05, 2021. https://ufdc.ufl.edu/AA00003837.

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

MLA Handbook (7th Edition):

Hoffmann, Sara Witherow. “Variations of the H and K emission lines of singly ionized calcium in the eclipsing binary star system AR Lacertae.” 1983. Web. 05 Mar 2021.

Vancouver:

Hoffmann SW. Variations of the H and K emission lines of singly ionized calcium in the eclipsing binary star system AR Lacertae. [Internet] [Thesis]. University of Florida; 1983. [cited 2021 Mar 05]. Available from: https://ufdc.ufl.edu/AA00003837.

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

Council of Science Editors:

Hoffmann SW. Variations of the H and K emission lines of singly ionized calcium in the eclipsing binary star system AR Lacertae. [Thesis]. University of Florida; 1983. Available from: https://ufdc.ufl.edu/AA00003837

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

22. McGill, Meghan A. Gravitational Darkening of Classical Be Stars.

Degree: 2013, University of Western Ontario

 Be stars are rapidly rotating B-type stars that possess a gaseous disk formed by matter released from the rapidly rotating, central star. The disk produces… (more)

Subjects/Keywords: Radiative transfer; circumstellar matter; Be stars; stellar rotation

…vertically-averaged, density-weighted temperature with disk radius for various stellar rotation… …5.1 Change in four disk temperature diagnostics with increasing stellar rotation and varying… …weighted temperature with disk radius for various stellar rotation rates and disk densities for… …radially-averaged temperature profile for various stellar rotation rates and disk densities for… …stellar effective temperatures including the effects of rotation versus rotation… 

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APA (6th Edition):

McGill, M. A. (2013). Gravitational Darkening of Classical Be Stars. (Thesis). University of Western Ontario. Retrieved from https://ir.lib.uwo.ca/etd/1256

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):

McGill, Meghan A. “Gravitational Darkening of Classical Be Stars.” 2013. Thesis, University of Western Ontario. Accessed March 05, 2021. https://ir.lib.uwo.ca/etd/1256.

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

MLA Handbook (7th Edition):

McGill, Meghan A. “Gravitational Darkening of Classical Be Stars.” 2013. Web. 05 Mar 2021.

Vancouver:

McGill MA. Gravitational Darkening of Classical Be Stars. [Internet] [Thesis]. University of Western Ontario; 2013. [cited 2021 Mar 05]. Available from: https://ir.lib.uwo.ca/etd/1256.

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

Council of Science Editors:

McGill MA. Gravitational Darkening of Classical Be Stars. [Thesis]. University of Western Ontario; 2013. Available from: https://ir.lib.uwo.ca/etd/1256

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

23. Simonian, Gregory Vahag Aghabekian. Double Trouble: The Impact of Binarity on Large Stellar Rotation Datasets.

Degree: PhD, Astronomy, 2019, The Ohio State University

 The Kepler satellite revolutionized our understanding of stellar rotation by providing tens of thousands of rotation periods for stars in the Kepler field, including a… (more)

Subjects/Keywords: Astronomy; stellar rotation; late-type stars; close binaries

stellar populations (Skumanich 1972), and correlations between rotation and age have… …studies of stellar rotation for cool stars have focused on young, solar metallicity clusters… …to measure stellar rotation in old field populations. Large-scale analyses have extracted… …stellar rotation. With the release of substantial rotation data with Kepler and APOGEE with the… …dependence of stellar rotation is that the rotation periods and metallicity must be measured… 

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APA (6th Edition):

Simonian, G. V. A. (2019). Double Trouble: The Impact of Binarity on Large Stellar Rotation Datasets. (Doctoral Dissertation). The Ohio State University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=osu1563439631310165

Chicago Manual of Style (16th Edition):

Simonian, Gregory Vahag Aghabekian. “Double Trouble: The Impact of Binarity on Large Stellar Rotation Datasets.” 2019. Doctoral Dissertation, The Ohio State University. Accessed March 05, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=osu1563439631310165.

MLA Handbook (7th Edition):

Simonian, Gregory Vahag Aghabekian. “Double Trouble: The Impact of Binarity on Large Stellar Rotation Datasets.” 2019. Web. 05 Mar 2021.

Vancouver:

Simonian GVA. Double Trouble: The Impact of Binarity on Large Stellar Rotation Datasets. [Internet] [Doctoral dissertation]. The Ohio State University; 2019. [cited 2021 Mar 05]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1563439631310165.

Council of Science Editors:

Simonian GVA. Double Trouble: The Impact of Binarity on Large Stellar Rotation Datasets. [Doctoral Dissertation]. The Ohio State University; 2019. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu1563439631310165


Georgia State University

24. Huang, Wenjin. Spectral Line Synthesis for Hot stars.

Degree: PhD, Physics and Astronomy, 2005, Georgia State University

 I developed a spectrum synthesis method to investigate the physical properties of hot OB main sequence (MS) stars, which are often rapid rotators. The code… (more)

Subjects/Keywords: Non-Radial Pulsation; Spectral Line Profiles; Spectrum Synthesis; Stellar Rotation; Massive Stars; Stellar Abundances; Galactic Clusters; Astrophysics and Astronomy; Physics

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APA (6th Edition):

Huang, W. (2005). Spectral Line Synthesis for Hot stars. (Doctoral Dissertation). Georgia State University. Retrieved from https://scholarworks.gsu.edu/phy_astr_diss/2

Chicago Manual of Style (16th Edition):

Huang, Wenjin. “Spectral Line Synthesis for Hot stars.” 2005. Doctoral Dissertation, Georgia State University. Accessed March 05, 2021. https://scholarworks.gsu.edu/phy_astr_diss/2.

MLA Handbook (7th Edition):

Huang, Wenjin. “Spectral Line Synthesis for Hot stars.” 2005. Web. 05 Mar 2021.

Vancouver:

Huang W. Spectral Line Synthesis for Hot stars. [Internet] [Doctoral dissertation]. Georgia State University; 2005. [cited 2021 Mar 05]. Available from: https://scholarworks.gsu.edu/phy_astr_diss/2.

Council of Science Editors:

Huang W. Spectral Line Synthesis for Hot stars. [Doctoral Dissertation]. Georgia State University; 2005. Available from: https://scholarworks.gsu.edu/phy_astr_diss/2

25. Chatzopoulos, Emmanouil. Superluminous supernovae : theory and observations.

Degree: PhD, Astronomy, 2013, University of Texas – Austin

 The discovery of superluminous supernovae in the past decade challenged our understanding of explosive stellar death. Subsequent extensive observations of superluminous supernova light curves and… (more)

Subjects/Keywords: Supernovae; Stellar evolution; Massive stars; Circumstellar matter; Light curve; Stellar rotation; Hydrodynamics

…mass stellar models for different degrees of ZAMS rotation. Filled black squares indicate… …Effects of Rotation on the Minimum Mass of Primordial Progenitors of Pair Instability… …xii 181 6.1 Characteristics of the stellar models discussed in this work. . . 7.1… …included in the calculations. The dotted lines mark the ZAMS mass and rotation level grid for the… …instability region as determined by the stellar equation of state. . . . . . 258 The internal… 

Page 1 Page 2 Page 3 Page 4 Page 5 Page 6 Page 7 Sample image

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APA (6th Edition):

Chatzopoulos, E. (2013). Superluminous supernovae : theory and observations. (Doctoral Dissertation). University of Texas – Austin. Retrieved from http://hdl.handle.net/2152/21758

Chicago Manual of Style (16th Edition):

Chatzopoulos, Emmanouil. “Superluminous supernovae : theory and observations.” 2013. Doctoral Dissertation, University of Texas – Austin. Accessed March 05, 2021. http://hdl.handle.net/2152/21758.

MLA Handbook (7th Edition):

Chatzopoulos, Emmanouil. “Superluminous supernovae : theory and observations.” 2013. Web. 05 Mar 2021.

Vancouver:

Chatzopoulos E. Superluminous supernovae : theory and observations. [Internet] [Doctoral dissertation]. University of Texas – Austin; 2013. [cited 2021 Mar 05]. Available from: http://hdl.handle.net/2152/21758.

Council of Science Editors:

Chatzopoulos E. Superluminous supernovae : theory and observations. [Doctoral Dissertation]. University of Texas – Austin; 2013. Available from: http://hdl.handle.net/2152/21758


University of Florida

26. Morgan, Thomas Harlow, 1945-. Fluid dynamics of circumstellar material associated with Be stars.

Degree: 1972, University of Florida

Subjects/Keywords: Approximation; Be stars; Coordinate systems; Emission spectra; Equations of motion; Mathematical variables; Stellar rotation; Stellar spectra; Time dependence; Velocity; B stars; Stars  – Atmospheres; Stars  – Spectra

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APA (6th Edition):

Morgan, Thomas Harlow, 1. (1972). Fluid dynamics of circumstellar material associated with Be stars. (Thesis). University of Florida. Retrieved from https://ufdc.ufl.edu/AA00011140

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):

Morgan, Thomas Harlow, 1945-. “Fluid dynamics of circumstellar material associated with Be stars.” 1972. Thesis, University of Florida. Accessed March 05, 2021. https://ufdc.ufl.edu/AA00011140.

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

MLA Handbook (7th Edition):

Morgan, Thomas Harlow, 1945-. “Fluid dynamics of circumstellar material associated with Be stars.” 1972. Web. 05 Mar 2021.

Vancouver:

Morgan, Thomas Harlow 1. Fluid dynamics of circumstellar material associated with Be stars. [Internet] [Thesis]. University of Florida; 1972. [cited 2021 Mar 05]. Available from: https://ufdc.ufl.edu/AA00011140.

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

Council of Science Editors:

Morgan, Thomas Harlow 1. Fluid dynamics of circumstellar material associated with Be stars. [Thesis]. University of Florida; 1972. Available from: https://ufdc.ufl.edu/AA00011140

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


University of Florida

27. Twigg, Laurence William, 1951- ( Dissertant ). An Analysis of the Rossiter effect in algol-type eclipsing binary systems.

Degree: 1979, University of Florida

One of the fundamental parameters of a star is its rate of axial

Subjects/Keywords: Eclipses; Eclipsing binary stars; Emission spectra; Hertzsprung Russell diagrams; Light curves; Radial velocity; Spectroscopy; Stellar classification; Stellar rotation; Velocity; Astronomy thesis Ph. D; Eclipsing binaries; Stars  – Rotation; Miami metropolitan area ( local )

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APA (6th Edition):

Twigg, Laurence William, 1. (. D. ). (1979). An Analysis of the Rossiter effect in algol-type eclipsing binary systems. (Thesis). University of Florida. Retrieved from https://ufdc.ufl.edu/UF00099116

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):

Twigg, Laurence William, 1951- ( Dissertant ). “An Analysis of the Rossiter effect in algol-type eclipsing binary systems.” 1979. Thesis, University of Florida. Accessed March 05, 2021. https://ufdc.ufl.edu/UF00099116.

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

MLA Handbook (7th Edition):

Twigg, Laurence William, 1951- ( Dissertant ). “An Analysis of the Rossiter effect in algol-type eclipsing binary systems.” 1979. Web. 05 Mar 2021.

Vancouver:

Twigg, Laurence William 1(D). An Analysis of the Rossiter effect in algol-type eclipsing binary systems. [Internet] [Thesis]. University of Florida; 1979. [cited 2021 Mar 05]. Available from: https://ufdc.ufl.edu/UF00099116.

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

Council of Science Editors:

Twigg, Laurence William 1(D). An Analysis of the Rossiter effect in algol-type eclipsing binary systems. [Thesis]. University of Florida; 1979. Available from: https://ufdc.ufl.edu/UF00099116

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


University of Florida

28. 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

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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


University of Florida

29. Davies, Chad Leslie, 1966-. Numerical modeling of large N galactic disk systems.

Degree: PhD, Physics, 1995, University of Florida

Subjects/Keywords: Angular momentum; Density; Galaxies; Galaxy rotation curves; Mass; Particle mass; Simulations; Star formation; Stellar disks; Velocity; Disks (Astrophysics)

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

APA (6th Edition):

Davies, Chad Leslie, 1. (1995). Numerical modeling of large N galactic disk systems. (Doctoral Dissertation). University of Florida. Retrieved from https://ufdc.ufl.edu/AA00058066

Chicago Manual of Style (16th Edition):

Davies, Chad Leslie, 1966-. “Numerical modeling of large N galactic disk systems.” 1995. Doctoral Dissertation, University of Florida. Accessed March 05, 2021. https://ufdc.ufl.edu/AA00058066.

MLA Handbook (7th Edition):

Davies, Chad Leslie, 1966-. “Numerical modeling of large N galactic disk systems.” 1995. Web. 05 Mar 2021.

Vancouver:

Davies, Chad Leslie 1. Numerical modeling of large N galactic disk systems. [Internet] [Doctoral dissertation]. University of Florida; 1995. [cited 2021 Mar 05]. Available from: https://ufdc.ufl.edu/AA00058066.

Council of Science Editors:

Davies, Chad Leslie 1. Numerical modeling of large N galactic disk systems. [Doctoral Dissertation]. University of Florida; 1995. Available from: https://ufdc.ufl.edu/AA00058066

.