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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 a 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, roč.~58, č.~5, s.~710-718. ISSN~0273-1177. Dostupné z: https://dx.doi.org/10.1016/j.asr.2016.01.002.
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