Multicomponent radiatively driven stellar winds. I. Nonisothermal three-component wind of hot B stars

Number of the records: 1

SYSNO ASEP	0124770
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Ostatní články
Title	Multicomponent radiatively driven stellar winds. I. Nonisothermal three-component wind of hot B stars
Author(s)	Krtička, Jiří (ASU-R) Kubát, Jiří (ASU-R)_{RID, ORCID}
Source Title	Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361 Roč. 369, č. 1 (2001), s. 222-238
Number of pages	17 s.
Language	eng - English
Country	FR - France
Keywords	hydrodynamics ; stars mass loss ; stars early type ; stars winds
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	KSK1003601 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
	KSK1043601 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
CEZ	AV0Z1003909 - ASU-R
Annotation	Nonisothermal winds of hot B stars are computed. Friction heats outer parts of the wind and modified temperature stratification ledds to a decrease of the outflow velocity.
Workplace	Astronomical Institute
Contact	Anežka Melichárková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2002

Number of the records: 1