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You searched for subject:(Magnetism Astrophysics ). Showing records 1 – 13 of 13 total matches.

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1. Rachmeler, L. A. Modeling eruptive coronal magnetohydrodynamic systems with FLUX.

Degree: 2010, University of Colorado at Boulder

  In this dissertation I explore solar coronal energetic eruptions in the context of magnetic reconnection, which is commonly thought to be a required trigger… (more)

Subjects/Keywords: Physics, Astrophysics; Physics, Electricity and Magnetism; Physics, Fluid and Plasma

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APA (6th Edition):

Rachmeler, L. A. (2010). Modeling eruptive coronal magnetohydrodynamic systems with FLUX. (Thesis). University of Colorado at Boulder. Retrieved from http://pqdtopen.proquest.com/#viewpdf?dispub=3404053

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):

Rachmeler, L A. “Modeling eruptive coronal magnetohydrodynamic systems with FLUX.” 2010. Thesis, University of Colorado at Boulder. Accessed December 03, 2020. http://pqdtopen.proquest.com/#viewpdf?dispub=3404053.

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

MLA Handbook (7th Edition):

Rachmeler, L A. “Modeling eruptive coronal magnetohydrodynamic systems with FLUX.” 2010. Web. 03 Dec 2020.

Vancouver:

Rachmeler LA. Modeling eruptive coronal magnetohydrodynamic systems with FLUX. [Internet] [Thesis]. University of Colorado at Boulder; 2010. [cited 2020 Dec 03]. Available from: http://pqdtopen.proquest.com/#viewpdf?dispub=3404053.

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

Council of Science Editors:

Rachmeler LA. Modeling eruptive coronal magnetohydrodynamic systems with FLUX. [Thesis]. University of Colorado at Boulder; 2010. Available from: http://pqdtopen.proquest.com/#viewpdf?dispub=3404053

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


Harvard University

2. Woolsey, Lauren. Magnetic Influences on the Solar Wind.

Degree: PhD, 2016, Harvard University

The steady, supersonic outflow from the Sun we call the solar wind was first posited in the 1950s and initial theories rightly linked the acceleration… (more)

Subjects/Keywords: Physics, Astronomy and Astrophysics; Physics, Electricity and Magnetism; Physics, Fluid and Plasma

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APA (6th Edition):

Woolsey, L. (2016). Magnetic Influences on the Solar Wind. (Doctoral Dissertation). Harvard University. Retrieved from http://nrs.harvard.edu/urn-3:HUL.InstRepos:33493537

Chicago Manual of Style (16th Edition):

Woolsey, Lauren. “Magnetic Influences on the Solar Wind.” 2016. Doctoral Dissertation, Harvard University. Accessed December 03, 2020. http://nrs.harvard.edu/urn-3:HUL.InstRepos:33493537.

MLA Handbook (7th Edition):

Woolsey, Lauren. “Magnetic Influences on the Solar Wind.” 2016. Web. 03 Dec 2020.

Vancouver:

Woolsey L. Magnetic Influences on the Solar Wind. [Internet] [Doctoral dissertation]. Harvard University; 2016. [cited 2020 Dec 03]. Available from: http://nrs.harvard.edu/urn-3:HUL.InstRepos:33493537.

Council of Science Editors:

Woolsey L. Magnetic Influences on the Solar Wind. [Doctoral Dissertation]. Harvard University; 2016. Available from: http://nrs.harvard.edu/urn-3:HUL.InstRepos:33493537

3. Lin, Jun. Theoretical mechanisms for solar eruptions.

Degree: PhD, 2001, University of New Hampshire

  This thesis presents new theoretical models of solar eruptions which are derived from older models that involve a loss of equilibrium of the Sun's… (more)

Subjects/Keywords: Physics; Astronomy and Astrophysics; Physics; Electricity and Magnetism

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APA (6th Edition):

Lin, J. (2001). Theoretical mechanisms for solar eruptions. (Doctoral Dissertation). University of New Hampshire. Retrieved from https://scholars.unh.edu/dissertation/41

Chicago Manual of Style (16th Edition):

Lin, Jun. “Theoretical mechanisms for solar eruptions.” 2001. Doctoral Dissertation, University of New Hampshire. Accessed December 03, 2020. https://scholars.unh.edu/dissertation/41.

MLA Handbook (7th Edition):

Lin, Jun. “Theoretical mechanisms for solar eruptions.” 2001. Web. 03 Dec 2020.

Vancouver:

Lin J. Theoretical mechanisms for solar eruptions. [Internet] [Doctoral dissertation]. University of New Hampshire; 2001. [cited 2020 Dec 03]. Available from: https://scholars.unh.edu/dissertation/41.

Council of Science Editors:

Lin J. Theoretical mechanisms for solar eruptions. [Doctoral Dissertation]. University of New Hampshire; 2001. Available from: https://scholars.unh.edu/dissertation/41


University of Colorado

4. Augustson, Kyle C. Convection and Dynamo Action in Massive Stars.

Degree: PhD, Astrophysical & Planetary Sciences, 2013, University of Colorado

  Contact between numerical simulations and observations of stellar magnetism is sought, with an emphasis on those stars that are the most readily observed and… (more)

Subjects/Keywords: Dynamo Theory; Fluid Dynamics; Stellar Convection; Stellar Magnetism; Astrophysics and Astronomy; Physical Processes; Stars, Interstellar Medium and the Galaxy

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APA (6th Edition):

Augustson, K. C. (2013). Convection and Dynamo Action in Massive Stars. (Doctoral Dissertation). University of Colorado. Retrieved from https://scholar.colorado.edu/astr_gradetds/26

Chicago Manual of Style (16th Edition):

Augustson, Kyle C. “Convection and Dynamo Action in Massive Stars.” 2013. Doctoral Dissertation, University of Colorado. Accessed December 03, 2020. https://scholar.colorado.edu/astr_gradetds/26.

MLA Handbook (7th Edition):

Augustson, Kyle C. “Convection and Dynamo Action in Massive Stars.” 2013. Web. 03 Dec 2020.

Vancouver:

Augustson KC. Convection and Dynamo Action in Massive Stars. [Internet] [Doctoral dissertation]. University of Colorado; 2013. [cited 2020 Dec 03]. Available from: https://scholar.colorado.edu/astr_gradetds/26.

Council of Science Editors:

Augustson KC. Convection and Dynamo Action in Massive Stars. [Doctoral Dissertation]. University of Colorado; 2013. Available from: https://scholar.colorado.edu/astr_gradetds/26


University of Florida

5. Wu, Benjamin. Giant Molecular Cloud Collisions as Triggers of Star Cluster Formation Numerical Simulations and Observational Predictions.

Degree: PhD, Physics, 2016, University of Florida

Stars primarily form in clusters from within giant molecular clouds (GMCs), but the dominant mechanisms triggering fragmentation and collapse are poorly understood. We Advisors/Committee Members: TAN,JONATHAN CHARLES (committee chair), WHITING,BERNARD F (committee member), LADA,ELIZABETH ANNE (committee member), GONZALEZ,ANTHONY HERNAN (committee member).

Subjects/Keywords: Average linear density; Cooling; Density; Heating; Magnetic fields; Magnetism; Magnets; Simulations; Star formation; Velocity; astronomy  – astrophysics  – numerical  – physics  – simulations  – star

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APA (6th Edition):

Wu, B. (2016). Giant Molecular Cloud Collisions as Triggers of Star Cluster Formation Numerical Simulations and Observational Predictions. (Doctoral Dissertation). University of Florida. Retrieved from https://ufdc.ufl.edu/UFE0050377

Chicago Manual of Style (16th Edition):

Wu, Benjamin. “Giant Molecular Cloud Collisions as Triggers of Star Cluster Formation Numerical Simulations and Observational Predictions.” 2016. Doctoral Dissertation, University of Florida. Accessed December 03, 2020. https://ufdc.ufl.edu/UFE0050377.

MLA Handbook (7th Edition):

Wu, Benjamin. “Giant Molecular Cloud Collisions as Triggers of Star Cluster Formation Numerical Simulations and Observational Predictions.” 2016. Web. 03 Dec 2020.

Vancouver:

Wu B. Giant Molecular Cloud Collisions as Triggers of Star Cluster Formation Numerical Simulations and Observational Predictions. [Internet] [Doctoral dissertation]. University of Florida; 2016. [cited 2020 Dec 03]. Available from: https://ufdc.ufl.edu/UFE0050377.

Council of Science Editors:

Wu B. Giant Molecular Cloud Collisions as Triggers of Star Cluster Formation Numerical Simulations and Observational Predictions. [Doctoral Dissertation]. University of Florida; 2016. Available from: https://ufdc.ufl.edu/UFE0050377

6. Tiedeken, Staci L. Magnetism and geology of the moon.

Degree: MS, Physics, 2017, University of Iowa

  Since different parts of the Moon display varying magnetic field strengths, our goal was to determine whether these differences are due to specific geological… (more)

Subjects/Keywords: Geology; Magnetism; Moon; Planetary science; Astrophysics and Astronomy

…36 3.2.2 Comparison to Magnetism… …global magnetic field and instead has extensive crustal magnetism. The average strength of the… …magnetism. The Lunar Prospector mission had the important tasks of recording gravity, magnetic… …lack of clear relationships between lunar magnetism and lunar geology. This absence of… …of very strong magnetism (Halekas et al., 2001). It has multiple origin stories… 

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APA (6th Edition):

Tiedeken, S. L. (2017). Magnetism and geology of the moon. (Masters Thesis). University of Iowa. Retrieved from https://ir.uiowa.edu/etd/5660

Chicago Manual of Style (16th Edition):

Tiedeken, Staci L. “Magnetism and geology of the moon.” 2017. Masters Thesis, University of Iowa. Accessed December 03, 2020. https://ir.uiowa.edu/etd/5660.

MLA Handbook (7th Edition):

Tiedeken, Staci L. “Magnetism and geology of the moon.” 2017. Web. 03 Dec 2020.

Vancouver:

Tiedeken SL. Magnetism and geology of the moon. [Internet] [Masters thesis]. University of Iowa; 2017. [cited 2020 Dec 03]. Available from: https://ir.uiowa.edu/etd/5660.

Council of Science Editors:

Tiedeken SL. Magnetism and geology of the moon. [Masters Thesis]. University of Iowa; 2017. Available from: https://ir.uiowa.edu/etd/5660


University of Arizona

7. Gibbard, Seran Gwen, 1967-. Lightning in the solar system .

Degree: 1996, University of Arizona

 Lightning, a familiar phenomenon on Earth, may also occur at other times and locations in our solar system. It has been suggested as a mechanism… (more)

Subjects/Keywords: Physics, Astronomy and Astrophysics.; Physics, Electricity and Magnetism.; Physics, Atmospheric Science.

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APA (6th Edition):

Gibbard, Seran Gwen, 1. (1996). Lightning in the solar system . (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/290640

Chicago Manual of Style (16th Edition):

Gibbard, Seran Gwen, 1967-. “Lightning in the solar system .” 1996. Doctoral Dissertation, University of Arizona. Accessed December 03, 2020. http://hdl.handle.net/10150/290640.

MLA Handbook (7th Edition):

Gibbard, Seran Gwen, 1967-. “Lightning in the solar system .” 1996. Web. 03 Dec 2020.

Vancouver:

Gibbard, Seran Gwen 1. Lightning in the solar system . [Internet] [Doctoral dissertation]. University of Arizona; 1996. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10150/290640.

Council of Science Editors:

Gibbard, Seran Gwen 1. Lightning in the solar system . [Doctoral Dissertation]. University of Arizona; 1996. Available from: http://hdl.handle.net/10150/290640


University of Arizona

8. Witczak, Steven Christopher, 1962-. Current gain degradation in bipolar junction transistors due to radiation, electrical and mechanical stresses .

Degree: 1996, University of Arizona

 The current gain of bipolar junction transistors is reduced due to ionizing radiation exposure or hot-carrier stressing. Radiation-induced degradation is particularly severe at the low… (more)

Subjects/Keywords: Engineering, Electronics and Electrical.; Physics, Astronomy and Astrophysics.; Physics, Electricity and Magnetism.; Physics, Radiation.

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APA (6th Edition):

Witczak, Steven Christopher, 1. (1996). Current gain degradation in bipolar junction transistors due to radiation, electrical and mechanical stresses . (Doctoral Dissertation). University of Arizona. Retrieved from http://hdl.handle.net/10150/282140

Chicago Manual of Style (16th Edition):

Witczak, Steven Christopher, 1962-. “Current gain degradation in bipolar junction transistors due to radiation, electrical and mechanical stresses .” 1996. Doctoral Dissertation, University of Arizona. Accessed December 03, 2020. http://hdl.handle.net/10150/282140.

MLA Handbook (7th Edition):

Witczak, Steven Christopher, 1962-. “Current gain degradation in bipolar junction transistors due to radiation, electrical and mechanical stresses .” 1996. Web. 03 Dec 2020.

Vancouver:

Witczak, Steven Christopher 1. Current gain degradation in bipolar junction transistors due to radiation, electrical and mechanical stresses . [Internet] [Doctoral dissertation]. University of Arizona; 1996. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/10150/282140.

Council of Science Editors:

Witczak, Steven Christopher 1. Current gain degradation in bipolar junction transistors due to radiation, electrical and mechanical stresses . [Doctoral Dissertation]. University of Arizona; 1996. Available from: http://hdl.handle.net/10150/282140


Indian Institute of Science

9. Chatterjee, Piyali. Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability.

Degree: PhD, Faculty of Science, 2010, Indian Institute of Science

 The Sun, by the virtue of its proximity to Earth, serves as an excellent astrophysical laboratory for testing our theoretical ideas. The Sun displays a… (more)

Subjects/Keywords: Solar Magnetic Field; Magnetism (Astrophysics); Helioseismology; Solar Dynamo Models; Solar Oscillations; Helicity; Solar Dynamo Theory; Stochastic Fluctuations; Mean Field Dynamo Model; Magnetic Flux Tube; Poloidal Field Accretion; Dynamo Model SURYA; Astrophysics

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APA (6th Edition):

Chatterjee, P. (2010). Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability. (Doctoral Dissertation). Indian Institute of Science. Retrieved from http://etd.iisc.ac.in/handle/2005/657

Chicago Manual of Style (16th Edition):

Chatterjee, Piyali. “Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability.” 2010. Doctoral Dissertation, Indian Institute of Science. Accessed December 03, 2020. http://etd.iisc.ac.in/handle/2005/657.

MLA Handbook (7th Edition):

Chatterjee, Piyali. “Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability.” 2010. Web. 03 Dec 2020.

Vancouver:

Chatterjee P. Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability. [Internet] [Doctoral dissertation]. Indian Institute of Science; 2010. [cited 2020 Dec 03]. Available from: http://etd.iisc.ac.in/handle/2005/657.

Council of Science Editors:

Chatterjee P. Understanding The Solar Magnetic Fields :Their Generation, Evolution And Variability. [Doctoral Dissertation]. Indian Institute of Science; 2010. Available from: http://etd.iisc.ac.in/handle/2005/657


Université de Montréal

10. Cossette, Jean-François. Simulations magnétohydrodynamiques en régime idéal.

Degree: 2015, Université de Montréal

Subjects/Keywords: Soleil; fluides; turbulence; magnétisme; irradiance; convection; reconnexion; simulation; semi-Lagrangien; Monge-Ampère; Sun; fluids; magnetism; reconnection; semi-Lagrangian; Physics - Astronomy and Astrophysics / Physique - Astronomie et astrophysique (UMI : 0606)

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APA (6th Edition):

Cossette, J. (2015). Simulations magnétohydrodynamiques en régime idéal. (Thesis). Université de Montréal. Retrieved from http://hdl.handle.net/1866/11672

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):

Cossette, Jean-François. “Simulations magnétohydrodynamiques en régime idéal.” 2015. Thesis, Université de Montréal. Accessed December 03, 2020. http://hdl.handle.net/1866/11672.

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

MLA Handbook (7th Edition):

Cossette, Jean-François. “Simulations magnétohydrodynamiques en régime idéal.” 2015. Web. 03 Dec 2020.

Vancouver:

Cossette J. Simulations magnétohydrodynamiques en régime idéal. [Internet] [Thesis]. Université de Montréal; 2015. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/1866/11672.

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

Council of Science Editors:

Cossette J. Simulations magnétohydrodynamiques en régime idéal. [Thesis]. Université de Montréal; 2015. Available from: http://hdl.handle.net/1866/11672

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

11. Thibault, Kim. Modélisation de l'évolution du réseau magnétique au cours du cycle solaire.

Degree: 2014, Université de Montréal

Subjects/Keywords: Soleil; Photosphère; Magnétisme; Activité solaire; Réseau magnétique; Simulation; Marche aléatoire; Sun; Photosphere; Magnetism; Solar activity; Magnetic network; Modelisation; Random walk; Physics - Astronomy and Astrophysics / Physique - Astronomie et astrophysique (UMI : 0606)

…couche situ´ ee au-dessus de la zone convective (Solar Astrophysics, Peter V. Foukal, 2004… …retournement est d’environ dix minutes (Solar Astrophysics, Peter V. Foukal, 2004, p.140)… …x28;Solar Astrophysics, Peter V. Foukal, 2004, p. 140). Leur diam` etre est estim´ e… 

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APA (6th Edition):

Thibault, K. (2014). Modélisation de l'évolution du réseau magnétique au cours du cycle solaire. (Thesis). Université de Montréal. Retrieved from http://hdl.handle.net/1866/11294

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):

Thibault, Kim. “Modélisation de l'évolution du réseau magnétique au cours du cycle solaire.” 2014. Thesis, Université de Montréal. Accessed December 03, 2020. http://hdl.handle.net/1866/11294.

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

MLA Handbook (7th Edition):

Thibault, Kim. “Modélisation de l'évolution du réseau magnétique au cours du cycle solaire.” 2014. Web. 03 Dec 2020.

Vancouver:

Thibault K. Modélisation de l'évolution du réseau magnétique au cours du cycle solaire. [Internet] [Thesis]. Université de Montréal; 2014. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/1866/11294.

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

Council of Science Editors:

Thibault K. Modélisation de l'évolution du réseau magnétique au cours du cycle solaire. [Thesis]. Université de Montréal; 2014. Available from: http://hdl.handle.net/1866/11294

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


ETH Zürich

12. Commichau, Sebastian Caspar. Observation of very high energy Gamma-rays from the Galactic Center with the MAGIC telescope, considering geomagnetic field effects on the imaging technique.

Degree: 2007, ETH Zürich

Subjects/Keywords: GAMMAASTROPHYSIK; MILCHSTRASSENZENTRUM (ASTRONOMIE); LUFTSCHAUEREXPERIMENTE (HOCHENERGIEPHYSIK); FEHLERRECHNUNG + AUSWERTUNG + INTERPRETATION (PHYSIK); ERDMAGNETISMUS + GEOMAGNETISMUS (GEOPHYSIK); GAMMA ASTROPHYSICS; GALACTIC CENTRE (ASTRONOMY); AIRSHOWER EXPERIMENTS (HIGH ENERGY PHYSICS); DATA EVALUATION + ERROR CALCULATION (PHYSICS); TERRESTRIAL MAGNETISM + GEOMAGNETISM (GEOPHYSICS); info:eu-repo/classification/ddc/520; info:eu-repo/classification/ddc/530; Astronomy, cartography; Physics

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APA (6th Edition):

Commichau, S. C. (2007). Observation of very high energy Gamma-rays from the Galactic Center with the MAGIC telescope, considering geomagnetic field effects on the imaging technique. (Doctoral Dissertation). ETH Zürich. Retrieved from http://hdl.handle.net/20.500.11850/149899

Chicago Manual of Style (16th Edition):

Commichau, Sebastian Caspar. “Observation of very high energy Gamma-rays from the Galactic Center with the MAGIC telescope, considering geomagnetic field effects on the imaging technique.” 2007. Doctoral Dissertation, ETH Zürich. Accessed December 03, 2020. http://hdl.handle.net/20.500.11850/149899.

MLA Handbook (7th Edition):

Commichau, Sebastian Caspar. “Observation of very high energy Gamma-rays from the Galactic Center with the MAGIC telescope, considering geomagnetic field effects on the imaging technique.” 2007. Web. 03 Dec 2020.

Vancouver:

Commichau SC. Observation of very high energy Gamma-rays from the Galactic Center with the MAGIC telescope, considering geomagnetic field effects on the imaging technique. [Internet] [Doctoral dissertation]. ETH Zürich; 2007. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/20.500.11850/149899.

Council of Science Editors:

Commichau SC. Observation of very high energy Gamma-rays from the Galactic Center with the MAGIC telescope, considering geomagnetic field effects on the imaging technique. [Doctoral Dissertation]. ETH Zürich; 2007. Available from: http://hdl.handle.net/20.500.11850/149899

13. Rolland, Benoit. Étude des propriétés atmosphériques et magnétiques des étoiles naines blanches froides riches en hydrogène.

Degree: 2014, Université de Montréal

Subjects/Keywords: Étoiles: naines blanches; Étoiles: paramètres fondamentaux; Étoiles: magnétisme; Modèles: atmosphère; Modèles: hydrogène; Techniques: photométrique et spectroscopique; Stars: white dwarfs; Stars: fundamental parameters; Stars: magnetism; Models: atmosphere; Models: hydrogen; Techniques: photometric and spectroscopic; Physics - Astronomy and Astrophysics / Physique - Astronomie et astrophysique (UMI : 0606)

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APA (6th Edition):

Rolland, B. (2014). Étude des propriétés atmosphériques et magnétiques des étoiles naines blanches froides riches en hydrogène. (Thesis). Université de Montréal. Retrieved from http://hdl.handle.net/1866/11105

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):

Rolland, Benoit. “Étude des propriétés atmosphériques et magnétiques des étoiles naines blanches froides riches en hydrogène.” 2014. Thesis, Université de Montréal. Accessed December 03, 2020. http://hdl.handle.net/1866/11105.

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

MLA Handbook (7th Edition):

Rolland, Benoit. “Étude des propriétés atmosphériques et magnétiques des étoiles naines blanches froides riches en hydrogène.” 2014. Web. 03 Dec 2020.

Vancouver:

Rolland B. Étude des propriétés atmosphériques et magnétiques des étoiles naines blanches froides riches en hydrogène. [Internet] [Thesis]. Université de Montréal; 2014. [cited 2020 Dec 03]. Available from: http://hdl.handle.net/1866/11105.

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

Council of Science Editors:

Rolland B. Étude des propriétés atmosphériques et magnétiques des étoiles naines blanches froides riches en hydrogène. [Thesis]. Université de Montréal; 2014. Available from: http://hdl.handle.net/1866/11105

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

.