The Influence of X-ray Emission on the Stellar Wind of O Stars
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216224%3A14310%2F08%3A00024794" target="_blank" >RIV/00216224:14310/08:00024794 - isvavai.cz</a>
Alternative codes found
RIV/67985815:_____/08:00318342
Result on the web
—
DOI - Digital Object Identifier
—
Alternative languages
Result language
angličtina
Original language name
The Influence of X-ray Emission on the Stellar Wind of O Stars
Original language description
We study the influence of X-ray radiation on the wind parameters of O stars. For this purpose we use our own NLTE wind code. The X-ray emission (assumed to be generated in wind shocks) is treated as an input quantity. We study its influence on the mass-loss rate, terminal velocity and ionization state of the stellar wind of Galactic O stars.
Czech name
Vliv rentgenového záření na hvězdný vítr O hvězd
Czech description
Studujeme vliv rentgenového záření na parametry větru O hvězd pomocí vlastních NLTE modelů větrů.
Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
—
Result continuities
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)
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
Mass Loss from Stars and the Evolution of Stellar Clusters
ISBN
978-1-58381-644-8
ISSN
—
e-ISSN
—
Number of pages
2
Pages from-to
—
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
—