Speaker
Mr
Jakub Fišák
(Masaryk University)
Description
There are many different opacity sources in the stellar atmospheres.
Because of limited computational time and memory the less important
opacity sources are usually neglected in stellar atmosphere models.
Rayleigh scattering is one of such opacities that are frequently neglected
in model atmospheres. But this neglect could not be valid for every case.
We study influence of the Rayleigh scattering by hydrogen, helium, and
selected metals on computed stellar atmospheres of hot stars with solar
chemical composition and some types of CP stars
Primary author
Mr
Jakub Fišák
(Masaryk University)
Co-authors
Dr
Dominik Munzar
(Masaryk University)
Prof.
Jiri Krticka
(Masaryk University)
Dr
Jiří Kubát
(Astronomical Institute of Academy of Sciences, Ondřejov)
