280505 VU PM-Astr The Physics of Galaxy Evolution (PI) (2017W)
Continuous assessment of course work
Labels
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).
- Registration is open from Th 14.09.2017 10:00 to Th 28.09.2017 23:59
- Registration is open from Tu 03.10.2017 10:00 to Th 19.10.2017 23:59
- Deregistration possible until Th 19.10.2017 23:59
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