Influence of the Frictional Heating on the Wind Line-Profiles of SMC Stars

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F08%3A00024795" target="_blank" >RIV/00216224:14310/08:00024795 - isvavai.cz</a>
Alternative codes found
RIV/67985815:_____/08:00321959
Result on the web
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DOI - Digital Object Identifier
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Result language
angličtina
Original language name
Influence of the Frictional Heating on the Wind Line-Profiles of SMC Stars
Original language description
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 transferequation 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 thisstar.
Czech name
Vliv ohřevu třením na profily čar z Malého Magellanova mračna
Czech description
Pomocí vlastních NLTE modelů studujeme vliv ohřevu třením na profily čar vznikajících ve hvězdném větru horkých hvězd Malého Magellanova mračna.

Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Publication year
2008
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Mass Loss from Stars and the Evolution of Stellar Clusters
ISBN
978-1-58381-644-8
ISSN
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e-ISSN
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Number of pages
2
Pages from-to
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Publisher name
Astronomical Society of the Pacific
Place of publication
San Francisco, USA
Event location
Lunteren, Nizozemí
Event date
Jan 1, 2006
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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