Magnetic B stars observed with BRITE: Spots, magnetospheres, binarity,   and pulsations
  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. 
G.A. Wade, D.H. Cohen, C. Fletcher, G. Handler, L. Huang, J. Krticka,   C. Neiner, E. Niemczura, H. Pablo, E. Paunzen, V. Pe...
astro-ph.SR