0124692 - ASU-R 20000151 RIV US eng C - Conference Paper (international conference)
Škoda, Petr - Koubský, Pavel
IUE spectra of Be star CX Dra: evidence for Winds.
The Be phenomenon in early-type stars. San Francisco: Astronomical Society of the Pacific, 2000 - (Smith, M.; Henrichs, H.; Fabregat, J.), s. 573-576
[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

The Be binary star CX Dra has been observed with the IUE satellite over a period of 14 years. After processing the quotient flux spectra of the Al III and Si IV lines show very complicated behaviour. The most important features are the violet shifted components in these lines which show very negative velocities in a particular phase interval.
Permanent Link: http://hdl.handle.net/11104/0022951