Stellar Atmospheres
Stockholm University
Startdatum:
Slutdatum:
Studietakt: 50 %
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Kod: AS7017
The course treats the physical principles of stellar atmospheres and methods for treating radiative transport in them. It takes up the basics for modelling such as continuum opacities, source functions, aspects of spectral line formation, curve of growth, as well as approximate methods such as Milne_Eddington, coherent scattering, non-LTE with complete redistribution and basic numerical methods. As a detailed example of relevant radiative processes it treats the VAL III model and its underlying physics.
To enter this course a Bachelor's degree in physics, or similar, is required. In addition, knowledge similar to the courses Stellar Structure and Evolution, 7.5 ECTS credits (AS7010) and Astrophysical Spectra, 7,5 ECTS credits (AS7006) is required. Swedish upper secondary school course English 6 or equivalent.
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Stockholm University
Startdatum:
Slutdatum:
Studietakt: 50 %
Hämtad: .
Publicerad: .
Publiceringsversion: 8e217193-f5fa-4778-b085-a4521fd03e8d
Kontrollsumma: 1b0dc54c0fc8a359f83ba9dc8f9d468479ce432de4c03bce3b8b33dd67fe3f6c
Senast ändrad enligt källan: 2025-08-25T09:20:11