Solens och Stjärnornas atmosfärer (Stellar Atmospheres), 5p HT 2002

The course will be given in English. Room: 63416

Lecturer: Paul Barklem (Room 63121, Ph 471 5981), Tutor: Michelle Mizuno (Room 63406, Ph 471 5992).

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 determination of a star 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. Includes fundamental observations, physical phenomena, modelling and comparison with observations.

Course Literature

Course requirements

Schedule

Day Date Time Class Please turn in
Tuesday Aug. 27 10:15 - 12:00
Lecture 1: Introduction
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Tuesday Sep. 3 10:15 - 12:00
Lecture 2: Radiative transfer
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Tuesday Sep. 10 10:15 - 12:00
Lecture 3: Opacity
Problem set 1
Tuesday Sep. 17 10:15 - 12:00
Lecture 4: Macrophysics
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Tuesday Sep. 24 10:15 - 12:00
Lecture 5: Line formation
Problem Set 2
Tuesday Oct. 1 10:15 - 12:00
Lecture 6: Stellar temperatures and gravities
Problem Set 3
Tuesday Oct. 8 10:15 - 12:00
Lecture 7: Chemical composition
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Tuesday Oct. 15 10:15 - 12:00
Lecture 8: Stellar winds
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Tuesday Oct. 22 10:15 - 12:00
Lecture 9: More realistic models
Lab report 1
Tuesday Oct. 29 10:15 - 12:00
Lecture 10: Observations
Lab report 2
Tuesday Nov. 5 10:15 - 12:00 Review Session
Monday Nov. 11 10:00 - 15:00 FINAL EXAM

Useful links


Paul Barklem
Michelle Mizuno-Wiedner
Last modified: Tue Mar 11 14:20:00 MET 2003