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280513 VU PM-Astr Cosmic Chemical Evolution (PI) (2022S)
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 08.02.2022 08:00 to We 23.02.2022 12:00
- Registration is open from Mo 28.02.2022 08:00 to Tu 15.03.2022 12:00
- Deregistration possible until Th 31.03.2022 23:59
Details
max. 20 participants
Language: German, English
Lecturers
Classes (iCal) - next class is marked with N
- Monday 07.03. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 14.03. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 21.03. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 28.03. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 04.04. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 25.04. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 02.05. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 09.05. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 16.05. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 23.05. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 30.05. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 13.06. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 20.06. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
- Monday 27.06. 11:30 - 13:00 Seminarraum 2 Astronomie Sternwarte, Türkenschanzstraße 17
Information
Aims, contents and method of the course
Assessment and permitted materials
An active participation and contributions are welcome.
Selected topics from the literature on nucleosynthesis, stellar mass loss, and galaxy evolution will be prepared by the students and presented to the participants.
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.
Presence in the courses of >75%, active contributions during the courxe, and self-sustained presentations of actual topics from the literature.
Presence in the courses of >75%, active contributions during the courxe, and self-sustained presentations of actual topics from the literature.
Examination topics
No separate exam, but questions from the context to be answered.
Reading list
Will be given during the lecture.
Association in the course directory
Last modified: Mo 07.03.2022 11:11
By means of stellar evolutionary models the nucleosynthesis of elements can be understood. Their release by various stellar mass-loss processes on different timescales enrich the interstellar medium (ISM) in its gas phases differently by these elements and, by this, the next stellar populations. Spectral observations of stars of different ages e.g. within the Mikly Way and in galaxies of variuos masses allow insights into timescales and amounts of element enrichments and though into the evolution of stellar and gaseous components. In addition, the observed ISM provides the actual chemical state which; however, is affected by gasdynamical effects.
Based on simple chemical evolutionary recipes, that include the so-called element yields, observational signatures of element abundances and abundance ratios will be studied and differences between galaxies compared with advanced dynamical evolutionary models.
The lecture will be held in English.