Magnetic B stars observed with BRITE: Spots, magnetospheres, binarity, and pulsations
G. A. Wade. Dept. of Physics , Royal Military College of Canada , CanadaDavid H. Cohen. Dept. of Physics and Astronomy , Swarthmore College , USAC. FletcherSpace Science InstituteG. Handler. Copernicus Astronomical Center , PolandHuang, L.. Dept. of Physics , Royal Military College of Canada , CanadaJiřı́ Krtička. Dept. of Theoretical Physics and Astrophysics , Masaryk University , Czech RepublicC. NeinerSorbonne UniversitéE. Niemczura. Astronomical Institute , University of Wroc law , Kopernika 11 , 51-622 Wroc law , PolandHerbert Pablo. Dépt. de Physique , Université de Montréal , CanadaE. Paunzen. Dept. of Theoretical Physics and Astrophysics , Masaryk University , Czech RepublicV. PétitSpace Science InstituteAndrzej Pigulski. Astronomical Institute , University of Wroc law , Kopernika 11 , 51-622 Wroc law , PolandTh. RiviniusJason F. Rowe. Dépt. de Physique , Université de Montréal , CanadaM. Rybicka. Copernicus Astronomical Center , PolandR. H. D. Townsend. Dept. of Astronomy , University of Wisconsin-Madison , USAMatt E. Shultz. Dept. of Physics , Engineering Physics and Astronomy , Queen's University , CanadaJ. Silvester. Uppsala University , SwedenJames Sikora. Dept. of Physics , Engineering Physics and Astronomy , Queen's University , Canada
2016en
ABI
Annotatsiya
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, $τ$ Sco, a Cen and $ε$ CMa.
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