Detailed Information on Publication Record
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
International impact
Změněno: 21/3/2018 23:21, Ing. Nicole Zrilić
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 |
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