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The triple B–star system DV Cam

Published online by Cambridge University Press:  25 February 2014

H. Hensberge
Affiliation:
Royal Observatory of Belgium, Brussels, Belgium
V. Bakış
Affiliation:
Akdeniz University, Faculty of Sciences, Department of Space Sciences and Technologies, Antalya, Turkey
P. De Cat
Affiliation:
Royal Observatory of Belgium, Brussels, Belgium
S. Bloemen
Affiliation:
Instituut voor Sterrenkunde, K.U. Leuven, Belgium
S. Scaringi
Affiliation:
Instituut voor Sterrenkunde, K.U. Leuven, Belgium
Á. Sódor
Affiliation:
Royal Observatory of Belgium, Brussels, Belgium
G. Raskin
Affiliation:
Instituut voor Sterrenkunde, K.U. Leuven, Belgium
H. Van Winckel
Affiliation:
Instituut voor Sterrenkunde, K.U. Leuven, Belgium
S. Prins
Affiliation:
Instituut voor Sterrenkunde, K.U. Leuven, Belgium
W. Pessemier
Affiliation:
Instituut voor Sterrenkunde, K.U. Leuven, Belgium
C. Waelkens
Affiliation:
Instituut voor Sterrenkunde, K.U. Leuven, Belgium
Y. Frémat
Affiliation:
Royal Observatory of Belgium, Brussels, Belgium
L. Dumortier
Affiliation:
Royal Observatory of Belgium, Brussels, Belgium
A. Jorissen
Affiliation:
Inst. d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Belgium
S. Van Eck
Affiliation:
Inst. d'Astronomie et d'Astrophysique, Université Libre de Bruxelles, Belgium
H. Lehmann
Affiliation:
Thüringer Landessternwarte Tautenburg (TLS), Germany
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Abstract

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.

Type
Research Article
Copyright
© EAS, EDP Sciences, 2014

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References

Bakış, V., Hensberge, H., Zejda, M., et al., 2011, Proc. IAU Symp., 282, 71CrossRef
Ilijić, S., 2003, MSc Thesis, Univ. Zagreb (http://sail.zpf.fer.hr/fdbinary/)
Lobel, A., 2011, Can. J. Phys., 89, 395CrossRef
Raskin, G., Van Winckel, H., Hensberge, H., et al., 2011, A&A, 526, A69

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