0469540 - ASÚ 2017 RIV GB eng J - Článek v odborném periodiku
Krtička, J. - Kubát, Jiří
Influence of X-ray radiation on the hot star wind ionization state and on the radiative force.
Advances in Space Research. Roč. 58, č. 5 (2016), s. 710-718. ISSN 0273-1177. E-ISSN 1879-1948
Institucionální podpora: RVO:67985815
Klíčová slova: Stars * winds * early-type stars
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika
Impakt faktor: 1.401, rok: 2016 ; AIS: 0.45, rok: 2016
DOI: https://doi.org/10.1016/j.asr.2016.01.002

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.
Trvalý link: http://hdl.handle.net/11104/0267320