D 2020

Ultraviolet variability of B, Be, and B[e] stars

KRTIČKOVÁ, Iva and Jiří KRTIČKA

Basic information

Original name

Ultraviolet variability of B, Be, and B[e] stars

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
Name: Ztráta hmoty v pozdních fázích vývoje hmotných hvězd
Investor: Czech Science Foundation