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Astrophysics III
Last Updated: 2026-06-03 00:14:41
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. Emphasis is put on general physical processes applicable in stellar physics and planet formation 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 Milky Way origin and evolution. - Physics of Molecular clouds - Protoplanetary Disks - Planet formation - Exoplanet detection
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 from Physics Bachelor (BSc Regulation 2021) is eligible as an elective. To assign a category, leave the option "no category" and contact the Study Administration ( ) once you have received the credits.)
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Deep Track Courses (At least 20 credits must be completed within the deep track courses. Surplus credit points can be counted towards the electives.)
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Deep Track Planetary Science (These courses can be credited either as a specialization subject or as an elective subject.)
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