Uppsala universitet
 
 

Stellar atmospheres (Solens och stjärnornas atmosfärer), 10 hp

The course will be given in English. Room: 63133 (Tammsalen)

Lecturer: Andreas Korn (Room 63412, Phone 471 5994), Bengt Gustafsson (Room 63119, Phone 471 5959). 
Tutor: Wladimir Lyra (Room 63411, Phone 471 5994).

Course Description

The vast majority of light in the universe originates from stars. Therefore, understanding of stellar atmospheres is the basis of interpretation for virtually all astronomical observations. Almost every type of analysis, from age determinations of stars in the solar neighbourhood to determining the chemical composition of distant galaxies, requires understanding of stellar atmospheres. This course deals with analysis and modelling of such atmospheres. Fundamental observations, physical phenomena, modelling and comparison with observations are also covered.

Course Literature

  • Gray, D.F., The observation and analysis of stellar photospheres, Cambridge University Press 1992.
    The course will follow this book's presentation and notation.
    (Copies are in the library. Buy directly from Cambridge or compare prices elsewhere with pricerunner. Be sure to get the corrections.)

  • Rutten, R.J., Lecture notes on Radiative Transfer in Stellar Atmospheres
    These lecture notes are very thorough when it comes to detailed radiative transfer.
    (Photocopies can be purchased from the department. Don't worry about downloading and printing these huge files yourself.)
     
  • Böhm-Vitense, E., Introduction to stellar astrophysics (vol. 2), Cambridge University Press 1989.
    If you lack some of the basics, this is a good starting point.
    (Copies are in the library. Buy directly from Cambridge or compare prices elsewhere with pricerunner.)

Course requirements

Schedule

Day Date Time Class Please turn in
 Thursday Sept. 6 10:15 - 12:00
Lecture 1: Introduction
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 Thursday Sept. 13 10:15 - 12:00
Lecture 2: Radiative transfer
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Monday Sept. 24 10:15 - 12:00
Lecture 3: Opacity (BG)
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 Thursday Sept. 27 15:15 - 17:00
Tutorial 1
Problem set 1
Tuesday Oct. 2 14:15 - 16:00
Lecture 4: Macrophysics (BG)
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 Thursday Oct. 4 10:15 - 12:00
Lecture 5: Line formation
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 Thursday Oct. 4 15:15 - 17:00
Tutorial 2
Problem set 2
 Thursday Oct. 11 13:15 - 15:00
Lecture 6: Stellar temperatures and gravities
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Tuesday Oct. 16 15:15 - 17:00
Tutorial 3
Problem set 3
 Thursday Oct. 18 10:15 - 12:00
Lecture 7: Chemical composition
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Wednesday Oct. 23 10:15 - 12:00
Lecture 8: More realistic models
Lab report 1
Wednesday Oct. 31 10:15 - 12:00
Lecture 9: Observations and applications
Lab report 2
Thursday Nov. 1 15:15 - 17:00            Tutorial before the exam  
Monday Nov. 5 10:00 - 13:00 FINAL EXAM


Useful links


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Responsible for this page: Andreas Korn
Updated: 2007-10-03