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280509 VO Stellar evolution and population sythesis (NPI) (2014W)
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Details
Language: English
Examination dates
Lecturers
Classes
Immer VO+UE, in Englisch!
16/10 THURSDAY 15:00-18:00, SE2
17/10 FRIDAY 15:00-17:00, SE2
20/10 MONDAY 9:30-11:00, SE1
22/10 WEDNESDAY 15:00-17:00, SE1
23/10 THURSDAY 15:00-17:00, SE2
29/10 WEDNESDAY 15:00-17:00, SE1
30/10 THURSDAY 15:00-17:00, SE2
06/11 THURSDAY 16:00-18:00, SE2
07/11 FRIDAY 15:00-17:00, SE2
10/11 MONDAY 9:30-11:00, SE1
13/11 THURSDAY 16:00-17:00, SE2
14/11 FRIDAY 15:00-17:00, SE2
17/11 MONDAY 9:30-11:00, SE1
19/11 WEDNESDAY 15:00-17:00, SE1
20/11 THURSDAY 15:00-17:00, SE2
Information
Aims, contents and method of the course
Assessment and permitted materials
Minimum requirements and assessment criteria
(1)Present/repeat the basics of stellar structure and evolution and
(2)apply these to the synthesis of stellar populations: what determines the observed star counts as a function of magnitude and wavelength? How to model it? How to extract information from the model-data comparisons?
(2)apply these to the synthesis of stellar populations: what determines the observed star counts as a function of magnitude and wavelength? How to model it? How to extract information from the model-data comparisons?
Examination topics
Reading list
Association in the course directory
Last modified: Mo 07.09.2020 15:42
transport, Nuclear reactions)
Stellar Evolution (basic equations, Evolution before and during the main sequence, The Helium burning phase, Advanced evolution of low- and intermediate-mass stars, Pre-supernova evolution of massive stars, Supernova explosions)
Population Synthesis (From (L;Teff ) to magnitudes and colors, From evolutionary tracks to isochrones, From isochrones to star clusters, From star clusters to resolved galaxies,
Modeling a galaxy (the Milky Way) from the inside, How to consider binaries?, How to treat circumstellar dust and ionized gas?, Integrated spectra, Stochastic and surface brightness fluctuations, CMD- and spectra-reconstruction techniques)