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@inproceedings{770645,
author = {Krtička, Jiří and Korcakova, Daniela and Kubát, Jiří},
address = {San Francisco, USA},
booktitle = {Mass Loss from Stars and the Evolution of Stellar Clusters},
keywords = {Hydrodynamics - stars stars: mass-loss stars: early-type stars: winds line profiles},
language = {eng},
location = {San Francisco, USA},
isbn = {978-1-58381-644-8},
pages = {191-192},
publisher = {Astronomical Society of the Pacific},
title = {Influence of the Frictional Heating on the Wind Line-Profiles of SMC Stars},
url = {http://www.aspbooks.org/a/volumes/article_details/?paper_id=28677},
year = {2008}
}
TY - JOUR
ID - 770645
AU - Krtička, Jiří - Korcakova, Daniela - Kubát, Jiří
PY - 2008
TI - Influence of the Frictional Heating on the Wind Line-Profiles of SMC Stars
PB - Astronomical Society of the Pacific
CY - San Francisco, USA
SN - 9781583816448
KW - Hydrodynamics - stars stars: mass-loss stars: early-type stars: winds line profiles
UR - http://www.aspbooks.org/a/volumes/article_details/?paper_id=28677
N2 - We study the influence of the frictional heating on the wind line-profiles of SMC stars. For this purpose we use our NLTE wind code to obtain consistent occupation numbers of studied levels and our radiative transfer code to solve the radiative transfer equation in moving media. We compare predicted wind line profiles calculated with and without frictional heating for a low-luminosity SMC star with a weak wind and discuss the relevance of frictional heating as a solution of a weak-wind problem for this star.
ER -
KRTIČKA, Jiří, Daniela KORCAKOVA a Jiří KUBÁT. Influence of the Frictional Heating on the Wind Line-Profiles of SMC Stars. In \textit{Mass Loss from Stars and the Evolution of Stellar Clusters}. San Francisco, USA: Astronomical Society of the Pacific, 2008, s.~191-192. ISBN~978-1-58381-644-8.
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