Detailed Information on Publication Record
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
KRTIČKOVÁ, Iva and Jiří KRTIČKA
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
Stať ve sborníku
Field of Study
10308 Astronomy
Country of publisher
Austria
Confidentiality degree
není předmětem státního či obchodního tajemství
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
Změněno: 18/12/2020 08:52, Mgr. Marie 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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