280502 VU PM-Astr Galaxies and their Environments (PI) (2018S)
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 Tu 13.02.2018 10:00 to Tu 27.02.2018 23:59
- Registration is open from Fr 02.03.2018 00:00 to Th 22.03.2018 23:59
- Deregistration possible until Th 22.03.2018 23:59
Details
max. 15 participants
Language: English
Lecturers
Classes (iCal) - next class is marked with N
Monday
05.03.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
19.03.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
09.04.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
16.04.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
23.04.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
30.04.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
07.05.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
14.05.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
28.05.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
04.06.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
11.06.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
18.06.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Monday
25.06.
11:30 - 13:00
Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Information
Aims, contents and method of the course
Assessment and permitted materials
Presence during the lectures and self-sustained in-depth presentations of distinct topics from recent publications.
Minimum requirements and assessment criteria
presentation and 75% attendance
Examination topics
Reading list
will be assembled from recent literature
Association in the course directory
Last modified: Mo 07.09.2020 15:42
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 effects change their evolution and lead to morphological transformations. By this class we will study the environments of galaxies, different environmental effects, and their consequences on the evolution of galaxies of different masses.
The lecture will be held in German and/or English according to its needs!