WADE, G. A., D. H. COHEN, C. FLETCHER, G. HANDLER, L. HUANG, Jiří KRTIČKA, C. NEINER, E. NIEMCZURA, H. PABLO, Ernst PAUNZEN, V. PETIT, A. PIGULSKI, Th. RIVINIUS, J. ROWE, M. RYBICKA, R. TOWNSEND, M. SHULTZ, J. SILVESTER and J. SIKORA. Magnetic B stars observed with BRITE: Spots, magnetospheres, binarity, and pulsations. In BRITE. Second BRITE-Constellation Science Conference: Small satellites—big science. 5th ed. Warszawa: Polish Astronomical Society, 2017, p. 94-100. ISBN 978-83-938279-6-1.
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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
Original language Czech
Type of outcome Proceedings paper
Field of Study 10300 1.3 Physical sciences
Country of publisher Poland
Confidentiality degree is not subject to a state or trade secret
Publication form printed version "print"
WWW URL
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 NZ, rivok
Tags International impact
Changed by Changed by: Ing. Nicole Zrilić, učo 240776. Changed: 21/3/2018 23:21.
Abstract
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.
Abstract (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 projectName: Atmosféry a okolohvězdné prostředí magnetických horkých hvězd
Investor: Czech Science Foundation
PrintDisplayed: 26/4/2024 21:25