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

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arxiv 1611.02793 v2 pith:FMLQEN6O submitted 2016-11-09 astro-ph.SR

G.A. Wade , D.H. Cohen , C. Fletcher , G. Handler , L. Huang , J. Krticka , C. Neiner , E. Niemczura
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H. Pablo E. Paunzen V. Petit A. Pigulski Th. Rivinius J. Rowe M. Rybicka R. Townsend M. Shultz J. Silvester J. Sikora
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keywords magneticb-typebriteepsilonstarsbinaritycausesconsequently
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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 4 magnetic B-type systems: $\epsilon$ Lupi, $\tau$ Sco, a Cen and $\epsilon$ CMa.

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