Universität Wien
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280521 VU PM-Astr Physics of galaxy evolution (PI) (2021S)

4.00 ECTS (2.00 SWS), SPL 28 - Erdwissenschaften, Meteorologie - Geophysik und
Continuous assessment of course work
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: German, English

Lecturers

Classes (iCal) - next class is marked with N

Digitale und eventuell hybride Durchführung der Lehre (Änderungen abhängig von Corona-Regelungen ab 2. Semesterhälfte).

  • Thursday 04.03. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 11.03. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 18.03. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 25.03. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 15.04. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 22.04. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 29.04. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 06.05. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 20.05. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 27.05. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 10.06. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 17.06. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
  • Thursday 24.06. 16:45 - 18:15 Digital
    Hybride Lehre
    Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17

Information

Aims, contents and method of the course

Galaxies are formed in regions of different densities in the universe by means of mass accumulation and, by this, their evolution is affected by the environment. In addition, their motion in the cosmos leads to mutual interaction and to agglomeration to denser regions, e.g. galaxy groups and clusters. Also these effects change their evolution secundarily and lead to morphological transformations. This lecture aims at studying in addition to the isolation evolution the different environmental effects and their implications to the evolution of galaxies of different masses.
Lectures and slides will be presented in English.

Assessment and permitted materials

Various topics selected from actual publications will be presented by the students and discussed among the participants.
A lively participation in the lectures and discussions is expected and will be weighted.

Minimum requirements and assessment criteria

This course is dedicated to master and PhD students with knowledge in extragalactic astrophysics.
Attendance of the lecture slots by 75% at minimum and at least one personal presentation of each participant will lead to a positive evaluation. Individual grades will depend on scientific input and found knowledge.

Examination topics

Reading list

will be provided during the course.

Association in the course directory

Last modified: Fr 12.05.2023 00:22