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@article{1350443,
author = {Krtička, Jiří and Kubát, Jiří},
article_number = {5},
doi = {http://dx.doi.org/10.1016/j.asr.2016.01.002},
keywords = {Stars: winds Outflows; Stars: mass-loss; Stars: early-type; Hydrodynamics; X-rays: stars},
language = {eng},
issn = {0273-1177},
journal = {Advances in Space Research},
title = {Influence of X-ray radiation on the hot star wind ionization state and on the radiative force},
url = {http://adsabs.harvard.edu/abs/2016AdSpR..58..710K},
volume = {58},
year = {2016}
}
TY - JOUR
ID - 1350443
AU - Krtička, Jiří - Kubát, Jiří
PY - 2016
TI - Influence of X-ray radiation on the hot star wind ionization state and on the radiative force
JF - Advances in Space Research
VL - 58
IS - 5
SP - 710-718
EP - 710-718
PB - Elsevier
SN - 02731177
KW - Stars: winds Outflows
KW - Stars: mass-loss
KW - Stars: early-type
KW - Hydrodynamics
KW - X-rays: stars
UR - http://adsabs.harvard.edu/abs/2016AdSpR..58..710K
N2 - 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.
ER -
KRTIČKA, Jiří and Jiří KUBÁT. Influence of X-ray radiation on the hot star wind ionization state and on the radiative force. \textit{Advances in Space Research}. Elsevier, 2016, vol.~58, No~5, p.~710-718. ISSN~0273-1177. Available from: https://dx.doi.org/10.1016/j.asr.2016.01.002.
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