Universität Wien

280505 VU PM-Astr The Physics of Galaxy Evolution (PI) (2017W)

Continuous assessment of course work

Registration/Deregistration

Note: The time of your registration within the registration period has no effect on the allocation of places (no first come, first served).

Details

max. 15 participants
Language: English

Lecturers

Classes (iCal) - next class is marked with N

  • Monday 02.10. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 09.10. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 16.10. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 23.10. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 30.10. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 06.11. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 13.11. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 20.11. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 27.11. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 04.12. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 11.12. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 08.01. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 15.01. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 22.01. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 29.01. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 01.02. 11:30 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17

Information

Aims, contents and method of the course

Galaxies are formed in regions of diferent density in the universe and, by this, their evolution is affected by the original environment. In addition, their motion in the cosmos leads to mutual interaction and infall into denser regions, e.g. galaxy clusters. Also these efects change their evolution and leads to morphological transformations. By this class we will study the different environmental effects and their consequences on the evolution of galaxies of different masses.

Assessment and permitted materials

Participation at the lecture part and individual presentations of special subjects from the literature

Minimum requirements and assessment criteria

completed bachelor study in Astrophysics

Examination topics

Reading list


Association in the course directory

Last modified: Mo 07.09.2020 15:42