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You searched for subject:(Stars Rotation). Showing records 1 – 30 of 61 total matches.

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Columbia University

1. Nunez, Alejandro. The Relationship Between Stellar Rotation and Magnetic Activity as Revealed by M37 and Alpha Persei.

Degree: 2018, Columbia University

 In low-mass (≲1.2 M⊙) main-sequence stars, the combination of differential rotation and turbulent flows in the outer convective region generates strong magnetic fields. It has… (more)

Subjects/Keywords: Stars – Rotation; Stars – Magnetic fields; Low mass stars

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APA (6th Edition):

Nunez, A. (2018). The Relationship Between Stellar Rotation and Magnetic Activity as Revealed by M37 and Alpha Persei. (Doctoral Dissertation). Columbia University. Retrieved from https://doi.org/10.7916/D8V712F7

Chicago Manual of Style (16th Edition):

Nunez, Alejandro. “The Relationship Between Stellar Rotation and Magnetic Activity as Revealed by M37 and Alpha Persei.” 2018. Doctoral Dissertation, Columbia University. Accessed March 07, 2021. https://doi.org/10.7916/D8V712F7.

MLA Handbook (7th Edition):

Nunez, Alejandro. “The Relationship Between Stellar Rotation and Magnetic Activity as Revealed by M37 and Alpha Persei.” 2018. Web. 07 Mar 2021.

Vancouver:

Nunez A. The Relationship Between Stellar Rotation and Magnetic Activity as Revealed by M37 and Alpha Persei. [Internet] [Doctoral dissertation]. Columbia University; 2018. [cited 2021 Mar 07]. Available from: https://doi.org/10.7916/D8V712F7.

Council of Science Editors:

Nunez A. The Relationship Between Stellar Rotation and Magnetic Activity as Revealed by M37 and Alpha Persei. [Doctoral Dissertation]. Columbia University; 2018. Available from: https://doi.org/10.7916/D8V712F7


Vanderbilt University

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

Degree: PhD, Physics, 2012, Vanderbilt University

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

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

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APA (6th Edition):

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

Chicago Manual of Style (16th Edition):

Le Blanc, Thompson S. “The Role of Disks in the Angular Momentum Evolution of Young, Low-Mass Stars.” 2012. Doctoral Dissertation, Vanderbilt University. Accessed March 07, 2021. http://hdl.handle.net/1803/13325.

MLA Handbook (7th Edition):

Le Blanc, Thompson S. “The Role of Disks in the Angular Momentum Evolution of Young, Low-Mass Stars.” 2012. Web. 07 Mar 2021.

Vancouver:

Le Blanc TS. The Role of Disks in the Angular Momentum Evolution of Young, Low-Mass Stars. [Internet] [Doctoral dissertation]. Vanderbilt University; 2012. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/1803/13325.

Council of Science Editors:

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


Iowa State University

3. Bolie, Victor Wayne. Periodic orbits in the neighborhood of libration points in certain rotating systems.

Degree: 1952, Iowa State University

Subjects/Keywords: Stars – Rotation; Mathematics

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APA (6th Edition):

Bolie, V. W. (1952). Periodic orbits in the neighborhood of libration points in certain rotating systems. (Thesis). Iowa State University. Retrieved from https://lib.dr.iastate.edu/rtd/12905

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):

Bolie, Victor Wayne. “Periodic orbits in the neighborhood of libration points in certain rotating systems.” 1952. Thesis, Iowa State University. Accessed March 07, 2021. https://lib.dr.iastate.edu/rtd/12905.

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

MLA Handbook (7th Edition):

Bolie, Victor Wayne. “Periodic orbits in the neighborhood of libration points in certain rotating systems.” 1952. Web. 07 Mar 2021.

Vancouver:

Bolie VW. Periodic orbits in the neighborhood of libration points in certain rotating systems. [Internet] [Thesis]. Iowa State University; 1952. [cited 2021 Mar 07]. Available from: https://lib.dr.iastate.edu/rtd/12905.

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

Council of Science Editors:

Bolie VW. Periodic orbits in the neighborhood of libration points in certain rotating systems. [Thesis]. Iowa State University; 1952. Available from: https://lib.dr.iastate.edu/rtd/12905

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


University of British Columbia

4. Woods, David. Luminosity - velocity diagrams of virgo cluster spiral galaxies.

Degree: MS- MSc, Geophysics, 1990, University of British Columbia

 Luminosity-velocity diagrams for 12 spiral galaxies in the Virgo cluster are presented. Optical rotation curves obtained for the innermost portions of eight galaxies, complemented with… (more)

Subjects/Keywords: Stars  – Luminosity function; Stars  – Rotation

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APA (6th Edition):

Woods, D. (1990). Luminosity - velocity diagrams of virgo cluster spiral galaxies. (Masters Thesis). University of British Columbia. Retrieved from http://hdl.handle.net/2429/29342

Chicago Manual of Style (16th Edition):

Woods, David. “Luminosity - velocity diagrams of virgo cluster spiral galaxies.” 1990. Masters Thesis, University of British Columbia. Accessed March 07, 2021. http://hdl.handle.net/2429/29342.

MLA Handbook (7th Edition):

Woods, David. “Luminosity - velocity diagrams of virgo cluster spiral galaxies.” 1990. Web. 07 Mar 2021.

Vancouver:

Woods D. Luminosity - velocity diagrams of virgo cluster spiral galaxies. [Internet] [Masters thesis]. University of British Columbia; 1990. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/2429/29342.

Council of Science Editors:

Woods D. Luminosity - velocity diagrams of virgo cluster spiral galaxies. [Masters Thesis]. University of British Columbia; 1990. Available from: http://hdl.handle.net/2429/29342


The Ohio State University

5. Sonneborn, George. A stability analysis of the equatorial regions of rapidly rotating B stars.

Degree: PhD, Graduate School, 1980, The Ohio State University

Subjects/Keywords: Physics; B stars; Stars – Rotation

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APA (6th Edition):

Sonneborn, G. (1980). A stability analysis of the equatorial regions of rapidly rotating B stars. (Doctoral Dissertation). The Ohio State University. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=osu148715118016362

Chicago Manual of Style (16th Edition):

Sonneborn, George. “A stability analysis of the equatorial regions of rapidly rotating B stars.” 1980. Doctoral Dissertation, The Ohio State University. Accessed March 07, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=osu148715118016362.

MLA Handbook (7th Edition):

Sonneborn, George. “A stability analysis of the equatorial regions of rapidly rotating B stars.” 1980. Web. 07 Mar 2021.

Vancouver:

Sonneborn G. A stability analysis of the equatorial regions of rapidly rotating B stars. [Internet] [Doctoral dissertation]. The Ohio State University; 1980. [cited 2021 Mar 07]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu148715118016362.

Council of Science Editors:

Sonneborn G. A stability analysis of the equatorial regions of rapidly rotating B stars. [Doctoral Dissertation]. The Ohio State University; 1980. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=osu148715118016362

6. Ahmed, Ahmed. Nitrogen Abundances in Early-Type Be Stars.

Degree: 2015, University of Western Ontario

 A sample of 26 Be stars from the Magnetism in Massive Stars (MiMeS) spectroscopic survey are analyzed for their photospheric nitrogen abundances in an effort… (more)

Subjects/Keywords: stars: abundances - stars: atmospheres -stars: rotation - radiative transfer -line: formation; Stars, Interstellar Medium and the Galaxy

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APA (6th Edition):

Ahmed, A. (2015). Nitrogen Abundances in Early-Type Be Stars. (Thesis). University of Western Ontario. Retrieved from https://ir.lib.uwo.ca/etd/3354

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):

Ahmed, Ahmed. “Nitrogen Abundances in Early-Type Be Stars.” 2015. Thesis, University of Western Ontario. Accessed March 07, 2021. https://ir.lib.uwo.ca/etd/3354.

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

MLA Handbook (7th Edition):

Ahmed, Ahmed. “Nitrogen Abundances in Early-Type Be Stars.” 2015. Web. 07 Mar 2021.

Vancouver:

Ahmed A. Nitrogen Abundances in Early-Type Be Stars. [Internet] [Thesis]. University of Western Ontario; 2015. [cited 2021 Mar 07]. Available from: https://ir.lib.uwo.ca/etd/3354.

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

Council of Science Editors:

Ahmed A. Nitrogen Abundances in Early-Type Be Stars. [Thesis]. University of Western Ontario; 2015. Available from: https://ir.lib.uwo.ca/etd/3354

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

7. 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 07, 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. 07 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 07]. 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


Universidade do Rio Grande do Norte

8. Maciel, Saulo Carneiro. Uma análise teórica da evolução da rotação estelar .

Degree: 2007, Universidade do Rio Grande do Norte

 In the past 50 years, large efforts have been made toward the understanding of the stellar evolution. In the observational context, large sets of precise… (more)

Subjects/Keywords: Rotação; Estrelas subgigantes; Estrelas gigantes; Análise teórica; Rotation; Subgiants stars; Giants stars; Theoretical analysis

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APA (6th Edition):

Maciel, S. C. (2007). Uma análise teórica da evolução da rotação estelar . (Thesis). Universidade do Rio Grande do Norte. Retrieved from http://repositorio.ufrn.br/handle/123456789/16525

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):

Maciel, Saulo Carneiro. “Uma análise teórica da evolução da rotação estelar .” 2007. Thesis, Universidade do Rio Grande do Norte. Accessed March 07, 2021. http://repositorio.ufrn.br/handle/123456789/16525.

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

MLA Handbook (7th Edition):

Maciel, Saulo Carneiro. “Uma análise teórica da evolução da rotação estelar .” 2007. Web. 07 Mar 2021.

Vancouver:

Maciel SC. Uma análise teórica da evolução da rotação estelar . [Internet] [Thesis]. Universidade do Rio Grande do Norte; 2007. [cited 2021 Mar 07]. Available from: http://repositorio.ufrn.br/handle/123456789/16525.

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

Council of Science Editors:

Maciel SC. Uma análise teórica da evolução da rotação estelar . [Thesis]. Universidade do Rio Grande do Norte; 2007. Available from: http://repositorio.ufrn.br/handle/123456789/16525

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

9. Pinçon, Charly. Du transport de moment cinétique par les ondes internes de gravité à l'heure de la sismologie stellaire : On the angular momentum transport by internal gravity waves at the time of asteroseismology.

Degree: Docteur es, Astronomie et Astrophysique, 2017, Paris Sciences et Lettres (ComUE)

 Les missions spatiales CoRoT (2006-2014) et Kepler (2009) ont procuré de nombreuses données sismiques pour des milliers d'étoiles de faible masse. L'analyse de ces données… (more)

Subjects/Keywords: Étoiles; Évolution; Rotation; Astérosismologie; Ondes; Hydrodynamique; Stars; Evolution; Rotation; Asteroseismology; Waves; Hydrodynamics; 520

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APA (6th Edition):

Pinçon, C. (2017). Du transport de moment cinétique par les ondes internes de gravité à l'heure de la sismologie stellaire : On the angular momentum transport by internal gravity waves at the time of asteroseismology. (Doctoral Dissertation). Paris Sciences et Lettres (ComUE). Retrieved from http://www.theses.fr/2017PSLEO009

Chicago Manual of Style (16th Edition):

Pinçon, Charly. “Du transport de moment cinétique par les ondes internes de gravité à l'heure de la sismologie stellaire : On the angular momentum transport by internal gravity waves at the time of asteroseismology.” 2017. Doctoral Dissertation, Paris Sciences et Lettres (ComUE). Accessed March 07, 2021. http://www.theses.fr/2017PSLEO009.

MLA Handbook (7th Edition):

Pinçon, Charly. “Du transport de moment cinétique par les ondes internes de gravité à l'heure de la sismologie stellaire : On the angular momentum transport by internal gravity waves at the time of asteroseismology.” 2017. Web. 07 Mar 2021.

Vancouver:

Pinçon C. Du transport de moment cinétique par les ondes internes de gravité à l'heure de la sismologie stellaire : On the angular momentum transport by internal gravity waves at the time of asteroseismology. [Internet] [Doctoral dissertation]. Paris Sciences et Lettres (ComUE); 2017. [cited 2021 Mar 07]. Available from: http://www.theses.fr/2017PSLEO009.

Council of Science Editors:

Pinçon C. Du transport de moment cinétique par les ondes internes de gravité à l'heure de la sismologie stellaire : On the angular momentum transport by internal gravity waves at the time of asteroseismology. [Doctoral Dissertation]. Paris Sciences et Lettres (ComUE); 2017. Available from: http://www.theses.fr/2017PSLEO009

10. 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 07, 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. 07 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 07]. 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


University of Alberta

11. Couture, Claudine. Orbital influence of the oscillations excited inside a rotating star in a binary system.

Degree: MS, Department of Physics, 2002, University of Alberta

Subjects/Keywords: Stars – Rotation.; Stars – Orbits.; Equations of motion.; Neutron stars.

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APA (6th Edition):

Couture, C. (2002). Orbital influence of the oscillations excited inside a rotating star in a binary system. (Masters Thesis). University of Alberta. Retrieved from https://era.library.ualberta.ca/files/dn39x313m

Chicago Manual of Style (16th Edition):

Couture, Claudine. “Orbital influence of the oscillations excited inside a rotating star in a binary system.” 2002. Masters Thesis, University of Alberta. Accessed March 07, 2021. https://era.library.ualberta.ca/files/dn39x313m.

MLA Handbook (7th Edition):

Couture, Claudine. “Orbital influence of the oscillations excited inside a rotating star in a binary system.” 2002. Web. 07 Mar 2021.

Vancouver:

Couture C. Orbital influence of the oscillations excited inside a rotating star in a binary system. [Internet] [Masters thesis]. University of Alberta; 2002. [cited 2021 Mar 07]. Available from: https://era.library.ualberta.ca/files/dn39x313m.

Council of Science Editors:

Couture C. Orbital influence of the oscillations excited inside a rotating star in a binary system. [Masters Thesis]. University of Alberta; 2002. Available from: https://era.library.ualberta.ca/files/dn39x313m

12. 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 07, 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. 07 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 07]. 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 Melbourne

13. PERALTA, CARLOS ANDRES. Superfluid spherical Couette flow and rotational irregularities in pulsars.

Degree: 2006, University of Melbourne

 Small amplitude rotational irregularities are observed in a number of rotation-powered pulsars. They fall into two classes: (i) glitches, defined as abrupt increases in the… (more)

Subjects/Keywords: dense matter; hydrodynamics; stars: interior; stars: neutron; stars: rotation

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APA (6th Edition):

PERALTA, C. A. (2006). Superfluid spherical Couette flow and rotational irregularities in pulsars. (Doctoral Dissertation). University of Melbourne. Retrieved from http://hdl.handle.net/11343/39224

Chicago Manual of Style (16th Edition):

PERALTA, CARLOS ANDRES. “Superfluid spherical Couette flow and rotational irregularities in pulsars.” 2006. Doctoral Dissertation, University of Melbourne. Accessed March 07, 2021. http://hdl.handle.net/11343/39224.

MLA Handbook (7th Edition):

PERALTA, CARLOS ANDRES. “Superfluid spherical Couette flow and rotational irregularities in pulsars.” 2006. Web. 07 Mar 2021.

Vancouver:

PERALTA CA. Superfluid spherical Couette flow and rotational irregularities in pulsars. [Internet] [Doctoral dissertation]. University of Melbourne; 2006. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/11343/39224.

Council of Science Editors:

PERALTA CA. Superfluid spherical Couette flow and rotational irregularities in pulsars. [Doctoral Dissertation]. University of Melbourne; 2006. Available from: http://hdl.handle.net/11343/39224

14. Harris, Amy. The kinematics of the outer Galactic disk from A and F stars.

Degree: PhD, 2019, University of Hertfordshire

 The kinematics of stars in the outer Galactic disk is poorly known. In addition to constraining the Galactic potential, knowledge of the motions of stars(more)

Subjects/Keywords: Astronomy; Astrophysics; Kinematics; Stars; Milky Way; Galaxy; galactic disk; rotation curve; young stars; massive stars; F stars; A stars; Dynamics; outer disk; Gaia; proper motion; radial velocity; spectroscopy

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APA (6th Edition):

Harris, A. (2019). The kinematics of the outer Galactic disk from A and F stars. (Doctoral Dissertation). University of Hertfordshire. Retrieved from http://hdl.handle.net/2299/22451

Chicago Manual of Style (16th Edition):

Harris, Amy. “The kinematics of the outer Galactic disk from A and F stars.” 2019. Doctoral Dissertation, University of Hertfordshire. Accessed March 07, 2021. http://hdl.handle.net/2299/22451.

MLA Handbook (7th Edition):

Harris, Amy. “The kinematics of the outer Galactic disk from A and F stars.” 2019. Web. 07 Mar 2021.

Vancouver:

Harris A. The kinematics of the outer Galactic disk from A and F stars. [Internet] [Doctoral dissertation]. University of Hertfordshire; 2019. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/2299/22451.

Council of Science Editors:

Harris A. The kinematics of the outer Galactic disk from A and F stars. [Doctoral Dissertation]. University of Hertfordshire; 2019. Available from: http://hdl.handle.net/2299/22451

15. Harris, Amy. The kinematics of the outer Galactic disk from A and F stars.

Degree: PhD, 2019, University of Hertfordshire

 The kinematics of stars in the outer Galactic disk is poorly known. In addition to constraining the Galactic potential, knowledge of the motions of stars(more)

Subjects/Keywords: Astronomy; Astrophysics; Kinematics; Stars; Milky Way; Galaxy; galactic disk; rotation curve; young stars; massive stars; F stars; A stars; Dynamics; outer disk; Gaia; proper motion; radial velocity; spectroscopy

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APA (6th Edition):

Harris, A. (2019). The kinematics of the outer Galactic disk from A and F stars. (Doctoral Dissertation). University of Hertfordshire. Retrieved from https://doi.org/10.18745/th.22451 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.802952

Chicago Manual of Style (16th Edition):

Harris, Amy. “The kinematics of the outer Galactic disk from A and F stars.” 2019. Doctoral Dissertation, University of Hertfordshire. Accessed March 07, 2021. https://doi.org/10.18745/th.22451 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.802952.

MLA Handbook (7th Edition):

Harris, Amy. “The kinematics of the outer Galactic disk from A and F stars.” 2019. Web. 07 Mar 2021.

Vancouver:

Harris A. The kinematics of the outer Galactic disk from A and F stars. [Internet] [Doctoral dissertation]. University of Hertfordshire; 2019. [cited 2021 Mar 07]. Available from: https://doi.org/10.18745/th.22451 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.802952.

Council of Science Editors:

Harris A. The kinematics of the outer Galactic disk from A and F stars. [Doctoral Dissertation]. University of Hertfordshire; 2019. Available from: https://doi.org/10.18745/th.22451 ; https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.802952

16. 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 07, 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. 07 Mar 2021.

Vancouver:

Potter AT. Rotation and magnetism in massive stars. [Internet] [Doctoral dissertation]. University of Cambridge; 2012. [cited 2021 Mar 07]. 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


University of Toronto

17. Kissin, Yevgeni. Properties of Stellar Remnants: Rotational and Magnetic Evolution of Their Progenitors.

Degree: PhD, 2017, University of Toronto

 The rotation and magnetic evolution of stars is examined in detail. Advection of angular momentum by convective plumes is a source of differential rotation, which… (more)

Subjects/Keywords: Black holes; Magnetic fields; Neutron stars; Rotation; White dwarfs; 0596

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

APA (6th Edition):

Kissin, Y. (2017). Properties of Stellar Remnants: Rotational and Magnetic Evolution of Their Progenitors. (Doctoral Dissertation). University of Toronto. Retrieved from http://hdl.handle.net/1807/80715

Chicago Manual of Style (16th Edition):

Kissin, Yevgeni. “Properties of Stellar Remnants: Rotational and Magnetic Evolution of Their Progenitors.” 2017. Doctoral Dissertation, University of Toronto. Accessed March 07, 2021. http://hdl.handle.net/1807/80715.

MLA Handbook (7th Edition):

Kissin, Yevgeni. “Properties of Stellar Remnants: Rotational and Magnetic Evolution of Their Progenitors.” 2017. Web. 07 Mar 2021.

Vancouver:

Kissin Y. Properties of Stellar Remnants: Rotational and Magnetic Evolution of Their Progenitors. [Internet] [Doctoral dissertation]. University of Toronto; 2017. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/1807/80715.

Council of Science Editors:

Kissin Y. Properties of Stellar Remnants: Rotational and Magnetic Evolution of Their Progenitors. [Doctoral Dissertation]. University of Toronto; 2017. Available from: http://hdl.handle.net/1807/80715


University of Cambridge

18. 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 · 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 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 07, 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. 07 Mar 2021.

Vancouver:

Potter AT. Rotation and magnetism in massive stars. [Internet] [Doctoral dissertation]. University of Cambridge; 2012. [cited 2021 Mar 07]. 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


The Ohio State University

19. 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 07, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=osu1531927526281553.

MLA Handbook (7th Edition):

Tayar, Jamie Nicole. “Rotation in Red Giants.” 2018. Web. 07 Mar 2021.

Vancouver:

Tayar JN. Rotation in Red Giants. [Internet] [Doctoral dissertation]. The Ohio State University; 2018. [cited 2021 Mar 07]. 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


University of Sydney

20. 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 07, 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. 07 Mar 2021.

Vancouver:

Li G. Asteroseismology of gamma Doradus stars with Kepler . [Internet] [Thesis]. University of Sydney; 2020. [cited 2021 Mar 07]. 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

21. Saulo Carneiro Maciel. Uma análise teórica da evolução da rotação estelar.

Degree: 2007, Universidade Federal do Rio Grande do Norte

Nos últimos cinqüenta anos, grandes esforços foram feitos no intuito de se entender a evolução estelar. No contexto observacional, medidas precisas da velocidade rotacional projetada… (more)

Subjects/Keywords: Rotação; Estrelas subgigantes; Estrelas gigantes; Análise teórica; Subgiants stars; ASTRONOMIA ESPACIAL; Rotation; Giants stars; Theoretical analysis

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APA (6th Edition):

Maciel, S. C. (2007). Uma análise teórica da evolução da rotação estelar. (Thesis). Universidade Federal do Rio Grande do Norte. Retrieved from http://bdtd.bczm.ufrn.br/tedesimplificado//tde_busca/arquivo.php?codArquivo=1502

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):

Maciel, Saulo Carneiro. “Uma análise teórica da evolução da rotação estelar.” 2007. Thesis, Universidade Federal do Rio Grande do Norte. Accessed March 07, 2021. http://bdtd.bczm.ufrn.br/tedesimplificado//tde_busca/arquivo.php?codArquivo=1502.

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

MLA Handbook (7th Edition):

Maciel, Saulo Carneiro. “Uma análise teórica da evolução da rotação estelar.” 2007. Web. 07 Mar 2021.

Vancouver:

Maciel SC. Uma análise teórica da evolução da rotação estelar. [Internet] [Thesis]. Universidade Federal do Rio Grande do Norte; 2007. [cited 2021 Mar 07]. Available from: http://bdtd.bczm.ufrn.br/tedesimplificado//tde_busca/arquivo.php?codArquivo=1502.

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

Council of Science Editors:

Maciel SC. Uma análise teórica da evolução da rotação estelar. [Thesis]. Universidade Federal do Rio Grande do Norte; 2007. Available from: http://bdtd.bczm.ufrn.br/tedesimplificado//tde_busca/arquivo.php?codArquivo=1502

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


University of Exeter

22. 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 07, 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. 07 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 07]. 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

23. Patten, Brian Michael. The evolution of rotation and activity in young open clusters : the zero-age main sequence.

Degree: PhD, 2009, University of Hawaii – Manoa

Microfiche.

x, 112 leaves, bound ill. (some col.) 29 cm

I have undertaken a program of ground- and space-based observations to measure photometric rotation periods… (more)

Subjects/Keywords: Cool stars  – Luminosity function; Cool stars  – Rotation

…for Ie 2602 Suspected Members........... 44 6 Rotation Data for Late-Type Stars in IC… …rotation rate and convective mixing rate. The braking of rotation in MS stars is therefore a… …measure rotation periods for solar-type stars in both clusters, and to measure coronal activity… …Chapter 3: Rotation at the ZAMS… …90 4.5 Long-Term Activity Cycles........................ 91 4.6 Lx versus Rotation… 

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

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APA (6th Edition):

Patten, B. M. (2009). The evolution of rotation and activity in young open clusters : the zero-age main sequence. (Doctoral Dissertation). University of Hawaii – Manoa. Retrieved from http://hdl.handle.net/10125/9356

Chicago Manual of Style (16th Edition):

Patten, Brian Michael. “The evolution of rotation and activity in young open clusters : the zero-age main sequence.” 2009. Doctoral Dissertation, University of Hawaii – Manoa. Accessed March 07, 2021. http://hdl.handle.net/10125/9356.

MLA Handbook (7th Edition):

Patten, Brian Michael. “The evolution of rotation and activity in young open clusters : the zero-age main sequence.” 2009. Web. 07 Mar 2021.

Vancouver:

Patten BM. The evolution of rotation and activity in young open clusters : the zero-age main sequence. [Internet] [Doctoral dissertation]. University of Hawaii – Manoa; 2009. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/10125/9356.

Council of Science Editors:

Patten BM. The evolution of rotation and activity in young open clusters : the zero-age main sequence. [Doctoral Dissertation]. University of Hawaii – Manoa; 2009. Available from: http://hdl.handle.net/10125/9356


University of Arizona

24. Fleming, Thomas Anthony. Optical analysis of an x-ray selected sample of stars.

Degree: 1988, University of Arizona

 I analyse an x-ray selected sample of 128 late-type (F-M) stars. These stars were identified as optical counterparts to serendipitous x-ray detections made by the… (more)

Subjects/Keywords: X-ray astronomy.; Stars  – Luminosity function.; Stars  – Rotation.

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APA (6th Edition):

Fleming, T. A. (1988). Optical analysis of an x-ray selected sample of stars. (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/184366

Chicago Manual of Style (16th Edition):

Fleming, Thomas Anthony. “Optical analysis of an x-ray selected sample of stars. ” 1988. Doctoral Dissertation, University of Arizona. Accessed March 07, 2021. http://hdl.handle.net/10150/184366.

MLA Handbook (7th Edition):

Fleming, Thomas Anthony. “Optical analysis of an x-ray selected sample of stars. ” 1988. Web. 07 Mar 2021.

Vancouver:

Fleming TA. Optical analysis of an x-ray selected sample of stars. [Internet] [Doctoral dissertation]. University of Arizona; 1988. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/10150/184366.

Council of Science Editors:

Fleming TA. Optical analysis of an x-ray selected sample of stars. [Doctoral Dissertation]. University of Arizona; 1988. Available from: http://hdl.handle.net/10150/184366

25. Gagnier, Damien. Dynamique des étoiles massives proches de la rotation critique : Dynamics of massive stars at rotation rates close to criticality.

Degree: Docteur es, Astrophysique, Sciences de l'Espace, Planétologie, 2020, Université Toulouse III – Paul Sabatier

La rotation joue un rôle majeur sur la dynamique, la structure et l'évolution séculaire des étoiles massives, souvent rotateurs rapides. Elle implique le mélange des… (more)

Subjects/Keywords: Étoiles massives; Rotation; Vents radiatifs; Dynamique des fluides astrophysiques; Massive stars; Rotation; Radiation-driven winds; Strophysical fluid dynamics

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APA (6th Edition):

Gagnier, D. (2020). Dynamique des étoiles massives proches de la rotation critique : Dynamics of massive stars at rotation rates close to criticality. (Doctoral Dissertation). Université Toulouse III – Paul Sabatier. Retrieved from http://www.theses.fr/2020TOU30159

Chicago Manual of Style (16th Edition):

Gagnier, Damien. “Dynamique des étoiles massives proches de la rotation critique : Dynamics of massive stars at rotation rates close to criticality.” 2020. Doctoral Dissertation, Université Toulouse III – Paul Sabatier. Accessed March 07, 2021. http://www.theses.fr/2020TOU30159.

MLA Handbook (7th Edition):

Gagnier, Damien. “Dynamique des étoiles massives proches de la rotation critique : Dynamics of massive stars at rotation rates close to criticality.” 2020. Web. 07 Mar 2021.

Vancouver:

Gagnier D. Dynamique des étoiles massives proches de la rotation critique : Dynamics of massive stars at rotation rates close to criticality. [Internet] [Doctoral dissertation]. Université Toulouse III – Paul Sabatier; 2020. [cited 2021 Mar 07]. Available from: http://www.theses.fr/2020TOU30159.

Council of Science Editors:

Gagnier D. Dynamique des étoiles massives proches de la rotation critique : Dynamics of massive stars at rotation rates close to criticality. [Doctoral Dissertation]. Université Toulouse III – Paul Sabatier; 2020. Available from: http://www.theses.fr/2020TOU30159

26. Evano, Benjamin. Analyse semiclassique des modes d'oscillation chaotiques dans les étoiles en rotation rapide : Semiclassical analysis of chaotic oscillation modes in rapidly rotating stars.

Degree: Docteur es, Astrophysique, sciences de l'espace, planétologie, 2019, Université Toulouse III – Paul Sabatier

L'astérosismologie permet d'obtenir des informations sur la structure interne des étoiles par l'étude de leurs pulsations. Parmi les cibles des satellites CoRot, Kepler ou Tess,… (more)

Subjects/Keywords: Étoiles en rotation; Ondes; Chaos classique; Chaos quantiques; Waves; Rotating stars; Classical chaos; Quantum chaos

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APA (6th Edition):

Evano, B. (2019). Analyse semiclassique des modes d'oscillation chaotiques dans les étoiles en rotation rapide : Semiclassical analysis of chaotic oscillation modes in rapidly rotating stars. (Doctoral Dissertation). Université Toulouse III – Paul Sabatier. Retrieved from http://www.theses.fr/2019TOU30173

Chicago Manual of Style (16th Edition):

Evano, Benjamin. “Analyse semiclassique des modes d'oscillation chaotiques dans les étoiles en rotation rapide : Semiclassical analysis of chaotic oscillation modes in rapidly rotating stars.” 2019. Doctoral Dissertation, Université Toulouse III – Paul Sabatier. Accessed March 07, 2021. http://www.theses.fr/2019TOU30173.

MLA Handbook (7th Edition):

Evano, Benjamin. “Analyse semiclassique des modes d'oscillation chaotiques dans les étoiles en rotation rapide : Semiclassical analysis of chaotic oscillation modes in rapidly rotating stars.” 2019. Web. 07 Mar 2021.

Vancouver:

Evano B. Analyse semiclassique des modes d'oscillation chaotiques dans les étoiles en rotation rapide : Semiclassical analysis of chaotic oscillation modes in rapidly rotating stars. [Internet] [Doctoral dissertation]. Université Toulouse III – Paul Sabatier; 2019. [cited 2021 Mar 07]. Available from: http://www.theses.fr/2019TOU30173.

Council of Science Editors:

Evano B. Analyse semiclassique des modes d'oscillation chaotiques dans les étoiles en rotation rapide : Semiclassical analysis of chaotic oscillation modes in rapidly rotating stars. [Doctoral Dissertation]. Université Toulouse III – Paul Sabatier; 2019. Available from: http://www.theses.fr/2019TOU30173


University of Pennsylvania

27. Gilhool, Steven. Spectroscopic Analysis Of Stellar Rotational Velocity At The Bottom Of The Main Sequence.

Degree: 2018, University of Pennsylvania

 This thesis presents analyses aimed at understanding the rotational properties of stars at the bottom of the main sequence. The evolution of stellar angular momentum… (more)

Subjects/Keywords: data analysis; infrared; low-mass stars; rotation; spectroscopy; statistics; Astrophysics and Astronomy

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APA (6th Edition):

Gilhool, S. (2018). Spectroscopic Analysis Of Stellar Rotational Velocity At The Bottom Of The Main Sequence. (Thesis). University of Pennsylvania. Retrieved from https://repository.upenn.edu/edissertations/3043

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):

Gilhool, Steven. “Spectroscopic Analysis Of Stellar Rotational Velocity At The Bottom Of The Main Sequence.” 2018. Thesis, University of Pennsylvania. Accessed March 07, 2021. https://repository.upenn.edu/edissertations/3043.

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

MLA Handbook (7th Edition):

Gilhool, Steven. “Spectroscopic Analysis Of Stellar Rotational Velocity At The Bottom Of The Main Sequence.” 2018. Web. 07 Mar 2021.

Vancouver:

Gilhool S. Spectroscopic Analysis Of Stellar Rotational Velocity At The Bottom Of The Main Sequence. [Internet] [Thesis]. University of Pennsylvania; 2018. [cited 2021 Mar 07]. Available from: https://repository.upenn.edu/edissertations/3043.

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

Council of Science Editors:

Gilhool S. Spectroscopic Analysis Of Stellar Rotational Velocity At The Bottom Of The Main Sequence. [Thesis]. University of Pennsylvania; 2018. Available from: https://repository.upenn.edu/edissertations/3043

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

28. Karageorgopoulos, Vasileios. Υπολογιστική σχετικιστική μελέτη των αστέρων νετρονίων με γενίκευση της μεθόδου των μετανευτώνειων προσεγγίσεων.

Degree: 2017, University of Patras; Πανεπιστήμιο Πατρών

 The main subject of the present PhD Thesis is the rotating relativistic polytropic models of neutron stars. The final purpose is to compute the physical… (more)

Subjects/Keywords: Αστέρες νετρονίων; Σχετικιστικά πολυτροπικά μοντέλα; Μετανευτώνειες προσεγγίσεις; Κρίσιμη περιστροφή; Ομοιόμορφη περιστροφή; ΔΙΑΦΟΡΙΚΗ ΠΕΡΙΣΤΡΟΦΗ; Αστέρες χαμαιλέοντες; Διαταρακτικές μέθοδοι; Στρατηγική του μιγαδικού επιπέδου; Neutron stars; General-relativistic polytropic models; Post-Newtonian approximation; Critical rotation; Uniform rotation; DIFFERENTIAL ROTATION; Chameleon stars; Perturbation methods; Complex plane strategy

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

APA (6th Edition):

Karageorgopoulos, V. (2017). Υπολογιστική σχετικιστική μελέτη των αστέρων νετρονίων με γενίκευση της μεθόδου των μετανευτώνειων προσεγγίσεων. (Thesis). University of Patras; Πανεπιστήμιο Πατρών. Retrieved from http://hdl.handle.net/10442/hedi/40229

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):

Karageorgopoulos, Vasileios. “Υπολογιστική σχετικιστική μελέτη των αστέρων νετρονίων με γενίκευση της μεθόδου των μετανευτώνειων προσεγγίσεων.” 2017. Thesis, University of Patras; Πανεπιστήμιο Πατρών. Accessed March 07, 2021. http://hdl.handle.net/10442/hedi/40229.

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

MLA Handbook (7th Edition):

Karageorgopoulos, Vasileios. “Υπολογιστική σχετικιστική μελέτη των αστέρων νετρονίων με γενίκευση της μεθόδου των μετανευτώνειων προσεγγίσεων.” 2017. Web. 07 Mar 2021.

Vancouver:

Karageorgopoulos V. Υπολογιστική σχετικιστική μελέτη των αστέρων νετρονίων με γενίκευση της μεθόδου των μετανευτώνειων προσεγγίσεων. [Internet] [Thesis]. University of Patras; Πανεπιστήμιο Πατρών; 2017. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/10442/hedi/40229.

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

Council of Science Editors:

Karageorgopoulos V. Υπολογιστική σχετικιστική μελέτη των αστέρων νετρονίων με γενίκευση της μεθόδου των μετανευτώνειων προσεγγίσεων. [Thesis]. University of Patras; Πανεπιστήμιο Πατρών; 2017. Available from: http://hdl.handle.net/10442/hedi/40229

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


Université de Montréal

29. Van Grootel, Valérie. Étude des étoiles de la branche horizontale extrême par l'astérosismologie.

Degree: 2008, Université de Montréal

Subjects/Keywords: Étoiles; Stars; Oscillations-Étoiles; Oscillations-Stars; Intérieurs-Étoiles; Interior-Stars; Sous-naines-Étoiles; Subdwarfs-Stars; Branche horizentale extrême-Étoiles; Extreme horizental branch-Stars; Binaires; Binaries; Serrées-Étoiles; Close-Stars; Rotation-Étoiles; Rotation-Stars; Évolution; Evolution

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

APA (6th Edition):

Van Grootel, V. (2008). Étude des étoiles de la branche horizontale extrême par l'astérosismologie. (Thesis). Université de Montréal. Retrieved from http://hdl.handle.net/1866/6415

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):

Van Grootel, Valérie. “Étude des étoiles de la branche horizontale extrême par l'astérosismologie.” 2008. Thesis, Université de Montréal. Accessed March 07, 2021. http://hdl.handle.net/1866/6415.

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

MLA Handbook (7th Edition):

Van Grootel, Valérie. “Étude des étoiles de la branche horizontale extrême par l'astérosismologie.” 2008. Web. 07 Mar 2021.

Vancouver:

Van Grootel V. Étude des étoiles de la branche horizontale extrême par l'astérosismologie. [Internet] [Thesis]. Université de Montréal; 2008. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/1866/6415.

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

Council of Science Editors:

Van Grootel V. Étude des étoiles de la branche horizontale extrême par l'astérosismologie. [Thesis]. Université de Montréal; 2008. Available from: http://hdl.handle.net/1866/6415

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

30. Jones, Jeremy W. The Ages of A-Stars.

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

Stars with spectral type `A' (also called A-type stars or just A-stars) are bright intermediate mass stars (∼1.5-2.5 M) that make up ∼1% of… (more)

Subjects/Keywords: Astronomy; stars: early-type; stars: evolution; stars: rotation; stars: fundamental parameters; techniques: interferometric

…Spectral Type: Our Brightest Stellar Neighbors . . . 1 1.1.1 The Rapid Rotation of A-Stars… …stars with masses ranging from 1.0 to 2.5 M and an angular rotation rate of either 0% (… …The Rapid Rotation of A-Stars In addition to being more luminous than stars like our Sun, A… …the stellar wind to slow down rotation (Matt et al. 2012, 2015). A-stars, being… …interactions from these close companions could be the cause of their slow rotation. Ap stars, on the… 

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

APA (6th Edition):

Jones, J. W. (2016). The Ages of A-Stars. (Doctoral Dissertation). Georgia State University. Retrieved from https://scholarworks.gsu.edu/phy_astr_diss/86

Chicago Manual of Style (16th Edition):

Jones, Jeremy W. “The Ages of A-Stars.” 2016. Doctoral Dissertation, Georgia State University. Accessed March 07, 2021. https://scholarworks.gsu.edu/phy_astr_diss/86.

MLA Handbook (7th Edition):

Jones, Jeremy W. “The Ages of A-Stars.” 2016. Web. 07 Mar 2021.

Vancouver:

Jones JW. The Ages of A-Stars. [Internet] [Doctoral dissertation]. Georgia State University; 2016. [cited 2021 Mar 07]. Available from: https://scholarworks.gsu.edu/phy_astr_diss/86.

Council of Science Editors:

Jones JW. The Ages of A-Stars. [Doctoral Dissertation]. Georgia State University; 2016. Available from: https://scholarworks.gsu.edu/phy_astr_diss/86

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