back to search
You will learn fundamental concepts of theoretical astrophysics, from the structure and dynamics of compact objects to stars and up to galaxies and galaxy clusters. In the end you will be able to apply physical principles (gravitation, hydrodynamics, radiative transfer, equations of state), derive simple scaling relations, and describe astrophysical examples such as white dwarfs, stellar evolution, accretion, and shock fronts.
No ratings for this module yet.
Only fill in the categories you can judge – for each one, either stars and text together or nothing at all.
Reviews are automatically checked before they are published.
Official page in TUMonline · Details are not binding.