Multicomponent stellar winds of B stars
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F08%3A00024723" target="_blank" >RIV/00216224:14310/08:00024723 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Multicomponent stellar winds of B stars
Original language description
We study multicomponent effects in the stellar winds of B type stars. For stars with highest mass-loss rates the usual one-component approach is sufficient. For stars with weaker winds multicomponent effects become important. For even less dense winds hydrogen and helium fall back on the stellar surface or even a pure metallic wind is possible.
Czech name
Vícesložkové větry hvězd spektrálního typu B
Czech description
Studujeme vícesložkov= hvězdné větry hvězd spektrálního typu B.
Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GA205%2F07%2F0031" target="_blank" >GA205/07/0031: Stellar winds of first stars in the Universe</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2008
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of the CP#AP Workshop
ISBN
0-07-085615-X
ISSN
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e-ISSN
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Number of pages
2
Pages from-to
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Publisher name
Astronomicky ustav SAV
Place of publication
Bratislava
Event location
Vídeň, Rakousko
Event date
Jan 1, 2007
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000256514000059