Universität Wien

280227 VO Star- and Planetformation (2010S)

n.Ü.

Details

max. 30 participants
Language: German

Lecturers

Classes

Currently no class schedule is known.

Information

Aims, contents and method of the course

Star formation is triggered by a gravitational collapse of an interstellar cloud but numerous physical processes like fragmentation, magnetic braking, shock waves, radiative transfer as well as ambipolar diffusion are necessary to form stars.

Assessment and permitted materials

Minimum requirements and assessment criteria

Examination topics

Reading list


Association in the course directory

M114, M115

Last modified: Mo 07.09.2020 15:42