2020
Ultraviolet variability of B, Be, and B[e] stars
KRTIČKOVÁ, Iva and Jiří KRTIČKABasic information
Original name
Ultraviolet variability of B, Be, and B[e] stars
Authors
Edition
Vienna, Stars and their variability observed from space, p. 435-436, 2 pp. 2020
Publisher
University of Vienna
Other information
Language
English
Type of outcome
Proceedings paper
Field of Study
10308 Astronomy
Country of publisher
Austria
Confidentiality degree
is not subject to a state or trade secret
Publication form
electronic version available online
References:
Organization unit
Faculty of Science
Keywords in English
stars: early-type; stars: emission-line; Be; stars: variables: general; stars: oscillations
Tags
International impact, Reviewed
Changed: 18/12/2020 08:52, Mgr. Marie Novosadová Šípková, DiS.
Abstract
V originále
We study the ultraviolet variability of evolved B[e], Be, and B stars from our Galaxy and from the Magellanic Clouds. We use IUE observations to derive fluxes of individual stars in the selected bands in the near-UV and far-UV regions. We diagnose the variability in the lines and the total flux variability. We discuss the origin of the UV light variability of studied stars. We detected pulsations in B[e] star HD 50138, LBV-type variations in HD 34664, and constant luminosity for a group of B[e] supergiants.
Links
GA18-05665S, research and development project |
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