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Astrophysics III
Last Updated: 2026-02-05 16:06:43
Abstract
Astrophysics III is a course in Galactic Astrophysics. It introduces the concepts of stellar populations, stellar dynamics, interstellar medium (ISM), and star formation for understanding the physics and phenomenology of the different components of the Milky Way galaxy.
Objective
The course should provide basic knowledge for research projects in the field of star formation and interstellar matter. A strong emphasis is put on radiation processes and the determination of physical parameters from observations.
Content
Astrophysics III: Galactic Astrophysics - components of the Milky Way: stars, ISM, dark matter, - dynamics of the Milky Way and of different subcomponents, - the physics of the interstellar medium, - star formation and feedback, and - the Milky Way origin and evolution.
Resources
Lecture Notes
A lecture script will be distributed.
General Information
- Language
- English
- Levels
- MSC
- Frequency
- Yearly recurring
Examination
- Type
- session examination
- Mode
- oral 30 minutes
Course Components
| Type | Title | Time & Place | Hours |
|---|---|---|---|
| lecture | Astrophysics III: Galactic Astrophysics |
|
3 h weekly |
| exercise | Astrophysics III: Galactic Astrophysics |
|
2 h weekly |
Offered In
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Core Courses (One Core Course in Experimental or Theoretical Physics from Physics Bachelor is eligible; however, this Core Course from Physics Bachelor cannot be used to compensate for the mandatory Core Course in Experimental or Theoretical Physics. For the category assignment keep the choice "no category" and take contact with the Study Administration ( ) after having received the credits.)
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