D 2017

Magnetic B stars observed with BRITE: Spots, magnetospheres, binarity, and pulsations

WADE, G. A., D. H. COHEN, C. FLETCHER, G. HANDLER, L. HUANG et. al.

Basic information

Original name

Magnetic B stars observed with BRITE: Spots, magnetospheres, binarity, and pulsations

Name (in English)

Magnetic B stars observed with BRITE: Spots, magnetospheres, binarity, and pulsations

Authors

WADE, G. A. (124 Canada), D. H. COHEN (840 United States of America), C. FLETCHER (840 United States of America), G. HANDLER (40 Austria), L. HUANG (124 Canada), Jiří KRTIČKA (203 Czech Republic, guarantor, belonging to the institution), C. NEINER (250 France), E. NIEMCZURA (616 Poland), H. PABLO (840 United States of America), Ernst PAUNZEN (40 Austria, belonging to the institution), V. PETIT (840 United States of America), A. PIGULSKI (616 Poland), Th. RIVINIUS (276 Germany), J. ROWE (840 United States of America), M. RYBICKA (616 Poland), R. TOWNSEND (826 United Kingdom of Great Britain and Northern Ireland), M. SHULTZ (124 Canada), J. SILVESTER (752 Sweden) and J. SIKORA (752 Sweden)

Edition

5. vyd. Warszawa, Second BRITE-Constellation Science Conference: Small satellites—big science, p. 94-100, 7 pp. 2017

Publisher

Polish Astronomical Society

Other information

Language

Czech

Type of outcome

Stať ve sborníku

Field of Study

10300 1.3 Physical sciences

Country of publisher

Poland

Confidentiality degree

není předmětem státního či obchodního tajemství

Publication form

printed version "print"

References:

RIV identification code

RIV/00216224:14310/17:00095489

Organization unit

Faculty of Science

ISBN

978-83-938279-6-1

Keywords in English

stars; magnetospheres; pulsations; spots; binarity

Tags

Tags

International impact
Změněno: 21/3/2018 23:21, Ing. Nicole Zrilić

Abstract

V originále

Magnetic B-type stars exhibit photometric variability due to diverse causes, and consequently on a variety of timescales. In this paper we describe interpretation of BRITE photometry and related ground-based observations of four magnetic B-type systems: eps Lupi, tau Sco, a Cen and eps CMa.

In English

Magnetic B-type stars exhibit photometric variability due to diverse causes, and consequently on a variety of timescales. In this paper we describe interpretation of BRITE photometry and related ground-based observations of four magnetic B-type systems: eps Lupi, tau Sco, a Cen and eps CMa.

Links

GA16-01116S, research and development project
Name: Atmosféry a okolohvězdné prostředí magnetických horkých hvězd
Investor: Czech Science Foundation