0124694 - ASU-R 20000153 RIV US eng C - Conference Paper (international conference)
Kubát, Jiří
NLTE model atmospheres of irradiated stars in B binaries.
The Be phenomenon in early-type stars. San Francisco: Astronomical Society of the Pacific, 2000 - (Smith, M.; Henrichs, H.; Fabregat, J.), s. 705-708
[Colloquium of the International Astronomical Union /175./. Alicante (ES), 28.06.1999-02.07.1999]
Institutional research plan: CEZ:AV0Z1003909
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics

Model atmospheres of B stars irradiated by their companion are calculated using our model atmosphere computer code under the assumption of hydrostatic, radiative, and statistical equilibrium. The external source of radiation is able to change the temperature structure of the outer atmospheric layers of B stars significantly.
Permanent Link: http://hdl.handle.net/11104/0022953