Hostname: page-component-745bb68f8f-s22k5 Total loading time: 0 Render date: 2025-02-11T19:46:41.990Z Has data issue: false hasContentIssue false
  • English
  • Français

The triple B–star system DV Cam

Published online by Cambridge University Press:  25 February 2014

H. Hensberge ,
V. Bakış ,
P. De Cat ,
S. Bloemen ,
S. Scaringi ,
Á. Sódor ,
G. Raskin ,
H. Van Winckel ,
S. Prins  and
W. Pessemier
...Show all authors
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
Get access

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
Information
European Astronomical Society Publications Series , Volume 64: Setting a New Standard in the Analysis of Binary Stars , 2013 , pp. 397 - 398
Copyright
© EAS, EDP Sciences, 2014

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

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