Magnetic B stars observed with BRITE: Spots, magnetospheres, binarity, and pulsations
arXiv:1611.02793
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: $ε$ Lupi, $Ï$ Sco, a Cen and $ε$ CMa.
7 pages, proceedings of the 3rd BRITE Science Meeting