Universität Wien

280517 VU PM-Astr Galaxies and their surroundings (PI) (2021W)

4.00 ECTS (2.00 SWS), SPL 28 - Erdwissenschaften, Meteorologie - Geophysik und
Continuous assessment of course work
MIXED
Moodle

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

The course will be held in ENGLISH!

  • Monday 04.10. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 11.10. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 18.10. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 25.10. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 08.11. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 15.11. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 22.11. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 29.11. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 06.12. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 13.12. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 10.01. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 17.01. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 24.01. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Monday 31.01. 13:15 - 14:45 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17

Information

Aims, contents and method of the course

Galaxies are formed and evolve in regions of different densities and are affected by their environments by mutual interactions. The galaxy motion in the cosmos also leads to mutual galaxy interactions and to galaxy assembly to massive complexes, like e.g. galaxy groups and clusters. These effects change the evolution of galaxies and lead to morphological transformations. In this course we will study the environments of galaxies, the different environmental effects, and their consequences on the evolution of galaxies of different masses.

Assessment and permitted materials

according to the fulfillment of the requirements

Minimum requirements and assessment criteria

Participation in the courses of >75%, active contributions during the courxe, and self-sustained presentations of actual topics from the literature.

Examination topics

Reading list

will be provided during the course

Association in the course directory

Last modified: Th 30.09.2021 13:30