EAS Publications Series
Volume 64, 2013Setting a New Standard in the Analysis of Binary Stars
|Page(s)||397 - 398|
|Published online||25 February 2014|
K. Pavlovski, A. Tkachenko and G. Torres (eds)
EAS Publications Series, 64 (2013) 397–398
The triple B–star system DV Cam
1 Royal Observatory of Belgium, Brussels, Belgium
2 Akdeniz University, Faculty of Sciences, Department of Space Sciences and Technologies, Antalya, Turkey
3 Instituut voor Sterrenkunde, K.U. Leuven, Belgium
4 Inst. d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Belgium
5 Thüringer Landessternwarte Tautenburg (TLS), Germany
DV Cam is a triple system showing the diversity of the physics of photospheres of B-type stars at a common age: an SPB star in a wide orbit around a close binary consisting of an ultra-slowly rotating helium-weak star and a much faster rotating mid-B star.
© EAS, EDP Sciences, 2014
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