Universität Wien

280523 SE PM-Astr Dynamics of Stellar Systems (PI) (2021W)

Continuous assessment of course work
MIXED

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. 25 participants
Language: English

Lecturers

Classes (iCal) - next class is marked with N

Aimed to be held in person. In case of COVID-19 restrictions we will move to online-mode. Further information will be announced at the beginning of the semester.

  • Wednesday 06.10. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 13.10. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 20.10. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 27.10. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 03.11. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 10.11. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 17.11. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 24.11. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 01.12. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 15.12. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 12.01. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 19.01. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
  • Wednesday 26.01. 13:15 - 14:45 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17

Information

Aims, contents and method of the course

This seminar encompasses the weekly meeting of the "Dynamics of Stellar Systems" research group at the Department of Astrophysics: https://www.univie.ac.at/dynamics/

The focus is on understanding the dynamical structure and evolution of stellar systems. In nearby galaxies and stellar clusters, the 'fossil records' of their formation are uncovered by constructing realistic dynamical models that fit their photometric and spectroscopic observations in detail. The latter include integral-field spectroscopy, observed motions and properties of individual stars, as well as (strong) gravitational lensing observations. 

Participants discuss recent scientific developments in this field of astrophysics in the form of reviews of publications (a.k.a. journal club), feedback from related international meetings, as well as informal presentations by participants.

Assessment and permitted materials

The assessment will be based on active participation, i.e., contributing to the discussions through asking questions and providing input.

Minimum requirements and assessment criteria

The meetings are in English. It is recommended that you have completed the second-semester course ‘Extragalactic Astronomy’ as background though highly motivated MSc students in their first year are also welcome. A minimum participation of 75% is required as well as at least one informal presentation.

Examination topics

Theoretical and observational advances in "Dynamics of Stellar Systems".

Reading list

Potential reading materials will be suggested in the meeting announcements.

Association in the course directory

Last modified: Th 30.09.2021 13:30