| Issue |
EAS Publications Series
Volume 64, 2013
Setting a New Standard in the Analysis of Binary Stars
|
|
|---|---|---|
| Page(s) | 397 - 398 | |
| Section | Posters | |
| DOI | https://doi.org/10.1051/eas/1364063 | |
| Published online | 25 February 2014 | |
Setting a New Standard in the Analysis of Binary Stars
K. Pavlovski, A. Tkachenko and G. Torres (eds)
EAS Publications Series, 64 (2013) 397–398
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