280513 VU PM-Astr Cosmic chemical evolution (PI) (2019W)
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 We 11.09.2019 10:00 to We 25.09.2019 23:59
- Registration is open from Tu 01.10.2019 10:00 to Tu 15.10.2019 23:59
- Deregistration possible until Tu 15.10.2019 23:59
Details
max. 25 participants
Language: English
Lecturers
Classes (iCal) - next class is marked with N
starting lecture on Oct. 1st
- Tuesday 01.10. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 08.10. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 15.10. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 22.10. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 29.10. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 05.11. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 12.11. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 19.11. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 26.11. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 03.12. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 10.12. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 17.12. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 07.01. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 14.01. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 21.01. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
- Thursday 23.01. 15:00 - 16:30 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Tuesday 28.01. 15:00 - 16:30 Seminarraum 1 Astronomie Sternwarte, Türkenschanzstraße 17
Information
Aims, contents and method of the course
Since shortly after the Big Bang only H, He, and a few lighter elements were produced, the further production of heavier elements in the stellar interior is responsible for the present-day element abundances. By means of stellar evolutionary models the nucleosynthesis of elements can be understood. Their release by various stellar mass-loss processes enrich the interstellar medium in its gas phases differently by these elements. The timescales and quantities of element enrichment and gasdynamical influences as well determine element abundances and abundance ratios, which can both be observed in stars of different ages e.g. in the Milky Way and nearby galaxies. With dynamical models only chemical signatures can provide a detailed insight into galaxy evolution.
Assessment and permitted materials
Selected topics from the literature on nucleosynthesis, stellar mass loss, and galaxy evolution will be prepared by the students and presented to the participants.
Minimum requirements and assessment criteria
Continuous attendance, one presentation at least, and lively participation.
Examination topics
Reading list
will be provided in the lecture
Association in the course directory
Last modified: Mo 07.09.2020 15:21