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You searched for subject:(Stellar Winds ). Showing records 1 – 17 of 17 total matches.

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Queens University

1. David-Uraz, Alexandre. Investigating the potential magnetic origin of wind variability in OB stars .

Degree: Physics, Engineering Physics and Astronomy, 2016, Queens University

 In this thesis, the origin of large-scale structures in hot star winds, believed to be responsible for the presence of discrete absorption components (DACs) in… (more)

Subjects/Keywords: astrophysics ; stellar winds ; massive stars

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

APA (6th Edition):

David-Uraz, A. (2016). Investigating the potential magnetic origin of wind variability in OB stars . (Thesis). Queens University. Retrieved from http://hdl.handle.net/1974/14445

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):

David-Uraz, Alexandre. “Investigating the potential magnetic origin of wind variability in OB stars .” 2016. Thesis, Queens University. Accessed March 07, 2021. http://hdl.handle.net/1974/14445.

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

MLA Handbook (7th Edition):

David-Uraz, Alexandre. “Investigating the potential magnetic origin of wind variability in OB stars .” 2016. Web. 07 Mar 2021.

Vancouver:

David-Uraz A. Investigating the potential magnetic origin of wind variability in OB stars . [Internet] [Thesis]. Queens University; 2016. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/1974/14445.

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

Council of Science Editors:

David-Uraz A. Investigating the potential magnetic origin of wind variability in OB stars . [Thesis]. Queens University; 2016. Available from: http://hdl.handle.net/1974/14445

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


Queens University

2. Shultz, Matthew. The Rotational Evolution and Magnetospheric Emission of the Magnetic Early B-type Stars .

Degree: Physics, Engineering Physics and Astronomy, 2016, Queens University

 How do the magnetic fields of massive stars evolve over time? Are their gyrochronological ages consistent with ages inferred from evolutionary tracks? Why do most… (more)

Subjects/Keywords: Stellar Winds ; Binary Stars ; Magnetospheres ; Massive Stars ; Magnetic Braking ; Stellar Magnetism ; Spectropolarimetry

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APA (6th Edition):

Shultz, M. (2016). The Rotational Evolution and Magnetospheric Emission of the Magnetic Early B-type Stars . (Thesis). Queens University. Retrieved from http://hdl.handle.net/1974/14691

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):

Shultz, Matthew. “The Rotational Evolution and Magnetospheric Emission of the Magnetic Early B-type Stars .” 2016. Thesis, Queens University. Accessed March 07, 2021. http://hdl.handle.net/1974/14691.

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

MLA Handbook (7th Edition):

Shultz, Matthew. “The Rotational Evolution and Magnetospheric Emission of the Magnetic Early B-type Stars .” 2016. Web. 07 Mar 2021.

Vancouver:

Shultz M. The Rotational Evolution and Magnetospheric Emission of the Magnetic Early B-type Stars . [Internet] [Thesis]. Queens University; 2016. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/1974/14691.

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

Council of Science Editors:

Shultz M. The Rotational Evolution and Magnetospheric Emission of the Magnetic Early B-type Stars . [Thesis]. Queens University; 2016. Available from: http://hdl.handle.net/1974/14691

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


University of Delaware

3. Kee, Nathaniel Dylan. Radiative ablation of disks around massive stars.

Degree: PhD, University of Delaware, Department of Physics and Astronomy, 2015, University of Delaware

 Hot, massive stars (spectral types O and B) have extreme luminosities (104 − 106L ) that drive strong stellar winds through UV line-scattering. Some massive… (more)

Subjects/Keywords: Stars  – Radiation.; Disks (Astrophysics); X-rays.; Stellar winds.

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APA (6th Edition):

Kee, N. D. (2015). Radiative ablation of disks around massive stars. (Doctoral Dissertation). University of Delaware. Retrieved from http://udspace.udel.edu/handle/19716/17601

Chicago Manual of Style (16th Edition):

Kee, Nathaniel Dylan. “Radiative ablation of disks around massive stars.” 2015. Doctoral Dissertation, University of Delaware. Accessed March 07, 2021. http://udspace.udel.edu/handle/19716/17601.

MLA Handbook (7th Edition):

Kee, Nathaniel Dylan. “Radiative ablation of disks around massive stars.” 2015. Web. 07 Mar 2021.

Vancouver:

Kee ND. Radiative ablation of disks around massive stars. [Internet] [Doctoral dissertation]. University of Delaware; 2015. [cited 2021 Mar 07]. Available from: http://udspace.udel.edu/handle/19716/17601.

Council of Science Editors:

Kee ND. Radiative ablation of disks around massive stars. [Doctoral Dissertation]. University of Delaware; 2015. Available from: http://udspace.udel.edu/handle/19716/17601


Queens University

4. Shultz, Matthew Eric. Magnetic fields and the variable wind of the early-type supergiant β Ori .

Degree: Physics, Engineering Physics and Astronomy, 2012, Queens University

 Supergiant stars of spectral types B and A are characterized by variable and structured winds, as revealed by variability of optical and ultraviolet spectral lines.… (more)

Subjects/Keywords: stellar winds ; Stars (magnetic) ; stars (early type) ; stars (supergiant) ; spectropolarimetry

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APA (6th Edition):

Shultz, M. E. (2012). Magnetic fields and the variable wind of the early-type supergiant β Ori . (Thesis). Queens University. Retrieved from http://hdl.handle.net/1974/7165

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):

Shultz, Matthew Eric. “Magnetic fields and the variable wind of the early-type supergiant β Ori .” 2012. Thesis, Queens University. Accessed March 07, 2021. http://hdl.handle.net/1974/7165.

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

MLA Handbook (7th Edition):

Shultz, Matthew Eric. “Magnetic fields and the variable wind of the early-type supergiant β Ori .” 2012. Web. 07 Mar 2021.

Vancouver:

Shultz ME. Magnetic fields and the variable wind of the early-type supergiant β Ori . [Internet] [Thesis]. Queens University; 2012. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/1974/7165.

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

Council of Science Editors:

Shultz ME. Magnetic fields and the variable wind of the early-type supergiant β Ori . [Thesis]. Queens University; 2012. Available from: http://hdl.handle.net/1974/7165

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

5. Puebla, Raul Eduardo Puebla. Síntese espectral detalhada de discos de acrescão com vento.

Degree: PhD, Astronomia, 2010, University of São Paulo

Neste trabalho foi desenvolvido um novo m´etodo de s´ntese espectral para modelar o disco de acres¸cao de vari´aveis catacl´smicas (VCs) nao magn´eticas. O principal objetivo… (more)

Subjects/Keywords: Accretions Disk; Cataclysmic Variables; Discos de Acresção; Stellar Winds; Variáveis Cataclísmicas; Ventos Estelares

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APA (6th Edition):

Puebla, R. E. P. (2010). Síntese espectral detalhada de discos de acrescão com vento. (Doctoral Dissertation). University of São Paulo. Retrieved from http://www.teses.usp.br/teses/disponiveis/14/14131/tde-28092010-152003/ ;

Chicago Manual of Style (16th Edition):

Puebla, Raul Eduardo Puebla. “Síntese espectral detalhada de discos de acrescão com vento.” 2010. Doctoral Dissertation, University of São Paulo. Accessed March 07, 2021. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-28092010-152003/ ;.

MLA Handbook (7th Edition):

Puebla, Raul Eduardo Puebla. “Síntese espectral detalhada de discos de acrescão com vento.” 2010. Web. 07 Mar 2021.

Vancouver:

Puebla REP. Síntese espectral detalhada de discos de acrescão com vento. [Internet] [Doctoral dissertation]. University of São Paulo; 2010. [cited 2021 Mar 07]. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-28092010-152003/ ;.

Council of Science Editors:

Puebla REP. Síntese espectral detalhada de discos de acrescão com vento. [Doctoral Dissertation]. University of São Paulo; 2010. Available from: http://www.teses.usp.br/teses/disponiveis/14/14131/tde-28092010-152003/ ;


Rice University

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

Degree: PhD, Natural Sciences, 2014, Rice University

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

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

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APA (6th Edition):

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

Chicago Manual of Style (16th Edition):

Cauley, Paul Wilson. “Diagnosing Mass Flows Around Herbig Ae/Be Stars.” 2014. Doctoral Dissertation, Rice University. Accessed March 07, 2021. http://hdl.handle.net/1911/87727.

MLA Handbook (7th Edition):

Cauley, Paul Wilson. “Diagnosing Mass Flows Around Herbig Ae/Be Stars.” 2014. Web. 07 Mar 2021.

Vancouver:

Cauley PW. Diagnosing Mass Flows Around Herbig Ae/Be Stars. [Internet] [Doctoral dissertation]. Rice University; 2014. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/1911/87727.

Council of Science Editors:

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


University of Texas – Austin

7. Tsang, Tsz Ho. Monte Carlo radiation hydrodynamics in the super-Eddington regime.

Degree: PhD, Astronomy, 2018, University of Texas – Austin

 In this dissertation, we present three projects addressing the dynamical importance of radiation in turbulent media with super-Eddington flux. Examples of such media are massive… (more)

Subjects/Keywords: Star formation; Stellar atmosphere; Radiation-driven winds; Radiation hydrodynamics; Numerical methods; Radiative transfer

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APA (6th Edition):

Tsang, T. H. (2018). Monte Carlo radiation hydrodynamics in the super-Eddington regime. (Doctoral Dissertation). University of Texas – Austin. Retrieved from http://hdl.handle.net/2152/69240

Chicago Manual of Style (16th Edition):

Tsang, Tsz Ho. “Monte Carlo radiation hydrodynamics in the super-Eddington regime.” 2018. Doctoral Dissertation, University of Texas – Austin. Accessed March 07, 2021. http://hdl.handle.net/2152/69240.

MLA Handbook (7th Edition):

Tsang, Tsz Ho. “Monte Carlo radiation hydrodynamics in the super-Eddington regime.” 2018. Web. 07 Mar 2021.

Vancouver:

Tsang TH. Monte Carlo radiation hydrodynamics in the super-Eddington regime. [Internet] [Doctoral dissertation]. University of Texas – Austin; 2018. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/2152/69240.

Council of Science Editors:

Tsang TH. Monte Carlo radiation hydrodynamics in the super-Eddington regime. [Doctoral Dissertation]. University of Texas – Austin; 2018. Available from: http://hdl.handle.net/2152/69240


University of Exeter

8. 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


Université de Grenoble

9. Lamberts-Marcade, Astrid. Simulations numériques de collisions de vents dans les systèmes binaires : Numerical simulations of colliding winds in binary systems.

Degree: Docteur es, Astrophysique et milieux dilues, 2012, Université de Grenoble

L'objectif de cette thèse est de comprendre la structure des binaires gamma, binaires à collision de vents composées d'une étoile massive et d'un pulsar jeune.… (more)

Subjects/Keywords: Simulations hydrodynamiques; Vents stellaires; Systèmes binaires; Instabilités; Hydrodynamical simulations; Stellar winds; Binary systems; Instabilities; Numerical relativity; Gamma-ray binaries

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APA (6th Edition):

Lamberts-Marcade, A. (2012). Simulations numériques de collisions de vents dans les systèmes binaires : Numerical simulations of colliding winds in binary systems. (Doctoral Dissertation). Université de Grenoble. Retrieved from http://www.theses.fr/2012GRENY038

Chicago Manual of Style (16th Edition):

Lamberts-Marcade, Astrid. “Simulations numériques de collisions de vents dans les systèmes binaires : Numerical simulations of colliding winds in binary systems.” 2012. Doctoral Dissertation, Université de Grenoble. Accessed March 07, 2021. http://www.theses.fr/2012GRENY038.

MLA Handbook (7th Edition):

Lamberts-Marcade, Astrid. “Simulations numériques de collisions de vents dans les systèmes binaires : Numerical simulations of colliding winds in binary systems.” 2012. Web. 07 Mar 2021.

Vancouver:

Lamberts-Marcade A. Simulations numériques de collisions de vents dans les systèmes binaires : Numerical simulations of colliding winds in binary systems. [Internet] [Doctoral dissertation]. Université de Grenoble; 2012. [cited 2021 Mar 07]. Available from: http://www.theses.fr/2012GRENY038.

Council of Science Editors:

Lamberts-Marcade A. Simulations numériques de collisions de vents dans les systèmes binaires : Numerical simulations of colliding winds in binary systems. [Doctoral Dissertation]. Université de Grenoble; 2012. Available from: http://www.theses.fr/2012GRENY038


University of Montana

10. Naylor, Jaylene R. A radiation-driven wind model for massive stars: The effects of non-isothermal and finite disk assumptions.

Degree: MS, 1999, University of Montana

Subjects/Keywords: Stellar winds.; Mass loss (Astrophysics); Stars Radiation.

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APA (6th Edition):

Naylor, J. R. (1999). A radiation-driven wind model for massive stars: The effects of non-isothermal and finite disk assumptions. (Masters Thesis). University of Montana. Retrieved from https://scholarworks.umt.edu/etd/8328

Chicago Manual of Style (16th Edition):

Naylor, Jaylene R. “A radiation-driven wind model for massive stars: The effects of non-isothermal and finite disk assumptions.” 1999. Masters Thesis, University of Montana. Accessed March 07, 2021. https://scholarworks.umt.edu/etd/8328.

MLA Handbook (7th Edition):

Naylor, Jaylene R. “A radiation-driven wind model for massive stars: The effects of non-isothermal and finite disk assumptions.” 1999. Web. 07 Mar 2021.

Vancouver:

Naylor JR. A radiation-driven wind model for massive stars: The effects of non-isothermal and finite disk assumptions. [Internet] [Masters thesis]. University of Montana; 1999. [cited 2021 Mar 07]. Available from: https://scholarworks.umt.edu/etd/8328.

Council of Science Editors:

Naylor JR. A radiation-driven wind model for massive stars: The effects of non-isothermal and finite disk assumptions. [Masters Thesis]. University of Montana; 1999. Available from: https://scholarworks.umt.edu/etd/8328


Rochester Institute of Technology

11. Montez, Rodolfo. X-rays from planetary nebulae: Unveiling wind collisions and binarity.

Degree: PhD, School of Physics and Astronomy (COS), 2010, Rochester Institute of Technology

 Planetary nebulae (PNe), the ionized, ejected envelopes of low- to intermediate-mass stars, are thought to be shaped by a nascent fast wind from the spent… (more)

Subjects/Keywords: Binary stars; Planetary nebula; Shocks; Stellar evolution; Stellar winds; X-rays

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APA (6th Edition):

Montez, R. (2010). X-rays from planetary nebulae: Unveiling wind collisions and binarity. (Doctoral Dissertation). Rochester Institute of Technology. Retrieved from https://scholarworks.rit.edu/theses/36

Chicago Manual of Style (16th Edition):

Montez, Rodolfo. “X-rays from planetary nebulae: Unveiling wind collisions and binarity.” 2010. Doctoral Dissertation, Rochester Institute of Technology. Accessed March 07, 2021. https://scholarworks.rit.edu/theses/36.

MLA Handbook (7th Edition):

Montez, Rodolfo. “X-rays from planetary nebulae: Unveiling wind collisions and binarity.” 2010. Web. 07 Mar 2021.

Vancouver:

Montez R. X-rays from planetary nebulae: Unveiling wind collisions and binarity. [Internet] [Doctoral dissertation]. Rochester Institute of Technology; 2010. [cited 2021 Mar 07]. Available from: https://scholarworks.rit.edu/theses/36.

Council of Science Editors:

Montez R. X-rays from planetary nebulae: Unveiling wind collisions and binarity. [Doctoral Dissertation]. Rochester Institute of Technology; 2010. Available from: https://scholarworks.rit.edu/theses/36


Universiteit Utrecht

12. Gent, Jeroen Ivar van. The Baldwin-effect in Wolf-Rayet stars.

Degree: 2000, Universiteit Utrecht

 This thesis investigates the Baldwin-effect in Wolf-Rayet (WR) stars. The Baldwin-effect is a correlation with negative slope between the equivalent width of spectral emission lines… (more)

Subjects/Keywords: Natuur- en Sterrenkunde; stars; stellar atmospheres; Wolf-Rayet stars; model atmospheres; emission lines; mass-loss; stellar winds; distances; spectra; astrophysics

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APA (6th Edition):

Gent, J. I. v. (2000). The Baldwin-effect in Wolf-Rayet stars. (Doctoral Dissertation). Universiteit Utrecht. Retrieved from http://dspace.library.uu.nl:8080/handle/1874/647

Chicago Manual of Style (16th Edition):

Gent, Jeroen Ivar van. “The Baldwin-effect in Wolf-Rayet stars.” 2000. Doctoral Dissertation, Universiteit Utrecht. Accessed March 07, 2021. http://dspace.library.uu.nl:8080/handle/1874/647.

MLA Handbook (7th Edition):

Gent, Jeroen Ivar van. “The Baldwin-effect in Wolf-Rayet stars.” 2000. Web. 07 Mar 2021.

Vancouver:

Gent JIv. The Baldwin-effect in Wolf-Rayet stars. [Internet] [Doctoral dissertation]. Universiteit Utrecht; 2000. [cited 2021 Mar 07]. Available from: http://dspace.library.uu.nl:8080/handle/1874/647.

Council of Science Editors:

Gent JIv. The Baldwin-effect in Wolf-Rayet stars. [Doctoral Dissertation]. Universiteit Utrecht; 2000. Available from: http://dspace.library.uu.nl:8080/handle/1874/647

13. Gent, Jeroen Ivar van. The Baldwin-effect in Wolf-Rayet stars.

Degree: 2000, University Utrecht

 This thesis investigates the Baldwin-effect in Wolf-Rayet (WR) stars. The Baldwin-effect is a correlation with negative slope between the equivalent width of spectral emission lines… (more)

Subjects/Keywords: stars; stellar atmospheres; Wolf-Rayet stars; model atmospheres; emission lines; mass-loss; stellar winds; distances; spectra; astrophysics

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APA (6th Edition):

Gent, J. I. v. (2000). The Baldwin-effect in Wolf-Rayet stars. (Doctoral Dissertation). University Utrecht. Retrieved from https://dspace.library.uu.nl/handle/1874/647 ; URN:NBN:NL:UI:10-1874-647 ; 1874/647 ; URN:NBN:NL:UI:10-1874-647 ; https://dspace.library.uu.nl/handle/1874/647

Chicago Manual of Style (16th Edition):

Gent, Jeroen Ivar van. “The Baldwin-effect in Wolf-Rayet stars.” 2000. Doctoral Dissertation, University Utrecht. Accessed March 07, 2021. https://dspace.library.uu.nl/handle/1874/647 ; URN:NBN:NL:UI:10-1874-647 ; 1874/647 ; URN:NBN:NL:UI:10-1874-647 ; https://dspace.library.uu.nl/handle/1874/647.

MLA Handbook (7th Edition):

Gent, Jeroen Ivar van. “The Baldwin-effect in Wolf-Rayet stars.” 2000. Web. 07 Mar 2021.

Vancouver:

Gent JIv. The Baldwin-effect in Wolf-Rayet stars. [Internet] [Doctoral dissertation]. University Utrecht; 2000. [cited 2021 Mar 07]. Available from: https://dspace.library.uu.nl/handle/1874/647 ; URN:NBN:NL:UI:10-1874-647 ; 1874/647 ; URN:NBN:NL:UI:10-1874-647 ; https://dspace.library.uu.nl/handle/1874/647.

Council of Science Editors:

Gent JIv. The Baldwin-effect in Wolf-Rayet stars. [Doctoral Dissertation]. University Utrecht; 2000. Available from: https://dspace.library.uu.nl/handle/1874/647 ; URN:NBN:NL:UI:10-1874-647 ; 1874/647 ; URN:NBN:NL:UI:10-1874-647 ; https://dspace.library.uu.nl/handle/1874/647


University of Toledo

14. Thompson, Gregory Brandon. Time-series Analysis of Line Profile Variability in Optical Spectra of ε Orionis.

Degree: PhD, Physics, 2009, University of Toledo

  The subject of this thesis is the time-series analysis of 130 échelle spectra of ε Ori obtained at Ritter Observatory on the campus of… (more)

Subjects/Keywords: Astronomy; Astrophysics; line profile variability; time-series analysis; massive stars; early-type stars; hot supergiants; stellar winds; stellar pulsations

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APA (6th Edition):

Thompson, G. B. (2009). Time-series Analysis of Line Profile Variability in Optical Spectra of ε Orionis. (Doctoral Dissertation). University of Toledo. Retrieved from http://rave.ohiolink.edu/etdc/view?acc_num=toledo1249511358

Chicago Manual of Style (16th Edition):

Thompson, Gregory Brandon. “Time-series Analysis of Line Profile Variability in Optical Spectra of ε Orionis.” 2009. Doctoral Dissertation, University of Toledo. Accessed March 07, 2021. http://rave.ohiolink.edu/etdc/view?acc_num=toledo1249511358.

MLA Handbook (7th Edition):

Thompson, Gregory Brandon. “Time-series Analysis of Line Profile Variability in Optical Spectra of ε Orionis.” 2009. Web. 07 Mar 2021.

Vancouver:

Thompson GB. Time-series Analysis of Line Profile Variability in Optical Spectra of ε Orionis. [Internet] [Doctoral dissertation]. University of Toledo; 2009. [cited 2021 Mar 07]. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=toledo1249511358.

Council of Science Editors:

Thompson GB. Time-series Analysis of Line Profile Variability in Optical Spectra of ε Orionis. [Doctoral Dissertation]. University of Toledo; 2009. Available from: http://rave.ohiolink.edu/etdc/view?acc_num=toledo1249511358


North-West University

15. Van den Heever, Stefanus Petrus. Numerical modelling of stellar winds for supernova progenitors / Stefanus Petrus van den Heever.

Degree: 2011, North-West University

 A two-dimensional hydrodynamic numerical model is extended and applied to simulate the interaction between stellar winds and the interstellar medium (ISM). In particular, the stellar(more)

Subjects/Keywords: Stellar winds; interstellar medium; O- and B-type stars; termination shock; astropause; supernova remnant; molecular cloud; stellêre winde; interstellêre medium; O en B-tipe sterre; terminasieskok; astropouse; supernova-res; molekulêre wolk

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APA (6th Edition):

Van den Heever, S. P. (2011). Numerical modelling of stellar winds for supernova progenitors / Stefanus Petrus van den Heever. (Thesis). North-West University. Retrieved from http://hdl.handle.net/10394/9719

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 den Heever, Stefanus Petrus. “Numerical modelling of stellar winds for supernova progenitors / Stefanus Petrus van den Heever. ” 2011. Thesis, North-West University. Accessed March 07, 2021. http://hdl.handle.net/10394/9719.

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

MLA Handbook (7th Edition):

Van den Heever, Stefanus Petrus. “Numerical modelling of stellar winds for supernova progenitors / Stefanus Petrus van den Heever. ” 2011. Web. 07 Mar 2021.

Vancouver:

Van den Heever SP. Numerical modelling of stellar winds for supernova progenitors / Stefanus Petrus van den Heever. [Internet] [Thesis]. North-West University; 2011. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/10394/9719.

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

Council of Science Editors:

Van den Heever SP. Numerical modelling of stellar winds for supernova progenitors / Stefanus Petrus van den Heever. [Thesis]. North-West University; 2011. Available from: http://hdl.handle.net/10394/9719

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


Université de Montréal

16. Ramiaramanantsoa, Tahina. Sur les origines photosphériques des structures dans les vents des étoiles chaudes et lumineuses.

Degree: 2018, Université de Montréal

Subjects/Keywords: Étoiles massives; Taches stellaires; Vents stellaires; Photométrie; Spectroscopie; Astérosismologie; Xi Persei; Zeta Puppis; V973 Scorpii; Massive stars; Starspots; Stellar winds; Photometry; Spectroscopy; Asteroseismology; Physics - Astronomy and Astrophysics / Physique - Astronomie et astrophysique (UMI : 0606)

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

APA (6th Edition):

Ramiaramanantsoa, T. (2018). Sur les origines photosphériques des structures dans les vents des étoiles chaudes et lumineuses. (Thesis). Université de Montréal. Retrieved from http://hdl.handle.net/1866/21152

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):

Ramiaramanantsoa, Tahina. “Sur les origines photosphériques des structures dans les vents des étoiles chaudes et lumineuses.” 2018. Thesis, Université de Montréal. Accessed March 07, 2021. http://hdl.handle.net/1866/21152.

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

MLA Handbook (7th Edition):

Ramiaramanantsoa, Tahina. “Sur les origines photosphériques des structures dans les vents des étoiles chaudes et lumineuses.” 2018. Web. 07 Mar 2021.

Vancouver:

Ramiaramanantsoa T. Sur les origines photosphériques des structures dans les vents des étoiles chaudes et lumineuses. [Internet] [Thesis]. Université de Montréal; 2018. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/1866/21152.

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

Council of Science Editors:

Ramiaramanantsoa T. Sur les origines photosphériques des structures dans les vents des étoiles chaudes et lumineuses. [Thesis]. Université de Montréal; 2018. Available from: http://hdl.handle.net/1866/21152

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


Université de Montréal

17. Carlos-Leblanc, Danny. Simulations Monte Carlo de régions d'interaction en corotation dans le vent d'étoiles chaudes.

Degree: 2019, Université de Montréal

Subjects/Keywords: Vents stellaires; étoiles massives; polarisation; structures à grande échelle; transfert radiatif; simulation Monte Carlo; méthode: numérique; Stellar winds; Massive stars; Methods: numerical; Polarization; Large-scale structures; Radiative transfer; Monte Carlo simulations; Physics - Astronomy and Astrophysics / Physique - Astronomie et astrophysique (UMI : 0606)

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

APA (6th Edition):

Carlos-Leblanc, D. (2019). Simulations Monte Carlo de régions d'interaction en corotation dans le vent d'étoiles chaudes. (Thesis). Université de Montréal. Retrieved from http://hdl.handle.net/1866/22717

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):

Carlos-Leblanc, Danny. “Simulations Monte Carlo de régions d'interaction en corotation dans le vent d'étoiles chaudes.” 2019. Thesis, Université de Montréal. Accessed March 07, 2021. http://hdl.handle.net/1866/22717.

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

MLA Handbook (7th Edition):

Carlos-Leblanc, Danny. “Simulations Monte Carlo de régions d'interaction en corotation dans le vent d'étoiles chaudes.” 2019. Web. 07 Mar 2021.

Vancouver:

Carlos-Leblanc D. Simulations Monte Carlo de régions d'interaction en corotation dans le vent d'étoiles chaudes. [Internet] [Thesis]. Université de Montréal; 2019. [cited 2021 Mar 07]. Available from: http://hdl.handle.net/1866/22717.

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

Council of Science Editors:

Carlos-Leblanc D. Simulations Monte Carlo de régions d'interaction en corotation dans le vent d'étoiles chaudes. [Thesis]. Université de Montréal; 2019. Available from: http://hdl.handle.net/1866/22717

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

.