Detailed Information on Publication Record
2016
Influence of X-ray radiation on the hot star wind ionization state and on the radiative force
KRTIČKA, Jiří and Jiří KUBÁTBasic information
Original name
Influence of X-ray radiation on the hot star wind ionization state and on the radiative force
Authors
KRTIČKA, Jiří (203 Czech Republic, guarantor, belonging to the institution) and Jiří KUBÁT (203 Czech Republic)
Edition
Advances in Space Research, Elsevier, 2016, 0273-1177
Other information
Language
English
Type of outcome
Článek v odborném periodiku
Field of Study
10308 Astronomy
Country of publisher
United Kingdom of Great Britain and Northern Ireland
Confidentiality degree
není předmětem státního či obchodního tajemství
References:
Impact factor
Impact factor: 1.401
RIV identification code
RIV/00216224:14310/16:00088046
Organization unit
Faculty of Science
UT WoS
000381535100004
Keywords in English
Stars: winds Outflows; Stars: mass-loss; Stars: early-type; Hydrodynamics; X-rays: stars
Tags
International impact, Reviewed
Změněno: 6/4/2017 20:41, Ing. Andrea Mikešková
Abstract
V originále
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.
Links
| GA13-10589S, research and development project |
|