NLTE models of line-driven stellar winds III. Influence of X-ray radiation on wind structure of O stars

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SYSNO ASEP	0333237
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	NLTE models of line-driven stellar winds III. Influence of X-ray radiation on wind structure of O stars
Title	NLTE modely zářením urychlovaných hvězdných větrů III. Vliv rentgenového záření na strukturu větru OB hvězd
Author(s)	Krtička, J. (CZ) Kubát, Jiří (ASU-R)_{RID, ORCID}
Source Title	Monthly Notices of the Royal Astronomical Society. - : Oxford University Press - ISSN 0035-8711 Roč. 394, č. 4 (2009), s. 2065-2079
Number of pages	15 s.
Language	eng - English
Country	GB - United Kingdom
Keywords	hydrodynamics ; early-type stars ; mass-loss stars
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	GA205/08/0003 GA ČR - Czech Science Foundation (CSF)
	KJB301630501 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000266549600029
DOI	10.1111/j.1365-2966.2009.14457.x
Annotation	We study the influence of X rays on the wind structure of selected O stars. For this purpose we use our non local thermodynamic equilibrium (NLTE) wind code with inclusion of additional artificial source of X rays, assumed to originate in the wind shocks. We show that the influence of shock X ray emission on wind mass loss rate is relatively small.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2010

Number of the records: 1