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

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Authors

WADE G. A. COHEN D. H. FLETCHER C. HANDLER G. HUANG L. KRTIČKA Jiří NEINER C. NIEMCZURA E. PABLO H. PAUNZEN Ernst PETIT V. PIGULSKI A. RIVINIUS Th. ROWE J. RYBICKA M. TOWNSEND R. SHULTZ M. SILVESTER J. SIKORA J.

Year of publication 2017
Type Article in Proceedings
Conference Second BRITE-Constellation Science Conference: Small satellites—big science
MU Faculty or unit

Faculty of Science

Citation
Web https://www.pta.edu.pl/proc/v5p1
Keywords stars; magnetospheres; pulsations; spots; binarity
Description 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.
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