Influence of X-ray radiation on the hot star wind ionization state and on the radiative force

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F16%3A00469540" target="_blank" >RIV/67985815:_____/16:00469540 - isvavai.cz</a>
Alternative codes found
RIV/00216224:14310/16:00088046
Result on the web
<a href="http://dx.doi.org/10.1016/j.asr.2016.01.002" target="_blank" >http://dx.doi.org/10.1016/j.asr.2016.01.002</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.asr.2016.01.002" target="_blank" >10.1016/j.asr.2016.01.002</a>

Result language
angličtina
Original language name
Influence of X-ray radiation on the hot star wind ionization state and on the radiative force
Original language description
Hot stars emit large amounts of X-rays, which are assumed to originate in the supersonic stellar wind. Part of the emitted X-rays is subsequently absorbed in the wind and influences its ionization state. Because hot star winds are driven radiatively, the modified ionization equilibrium affects the radiative force. We review the recent progress in modeling the influence of X-rays on the radiative equilibrium and on the radiative force. We focus particularly on single stars with X-rays produced in wind shocks and on binaries with massive components, which belong to the most luminous objects in X-rays.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Project
<a href="/en/project/GA13-10589S" target="_blank" >GA13-10589S: Mass loss in hot massive stars</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2016
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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