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The triple B–star system DV Cam

  • H. Hensberge (a1), V. Bakış (a2), P. De Cat (a1), S. Bloemen (a3), S. Scaringi (a3), Á. Sódor (a1), G. Raskin (a3), H. Van Winckel (a3), S. Prins (a3), W. Pessemier (a3), C. Waelkens (a3), Y. Frémat (a1), L. Dumortier (a1), A. Jorissen (a4), S. Van Eck (a4) and H. Lehmann (a5)...

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.

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References

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[1]1Bakış, V., Hensberge, H., Zejda, M., et al., 2011, Proc. IAU Symp., 282, 71
[2]2Ilijić, S., 2003, MSc Thesis, Univ. Zagreb (http://sail.zpf.fer.hr/fdbinary/)
[3]3Lobel, A., 2011, Can. J. Phys., 89, 395
[4]4Raskin, G., Van Winckel, H., Hensberge, H., et al., 2011, A&A, 526, A69

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The triple B–star system DV Cam

  • H. Hensberge (a1), V. Bakış (a2), P. De Cat (a1), S. Bloemen (a3), S. Scaringi (a3), Á. Sódor (a1), G. Raskin (a3), H. Van Winckel (a3), S. Prins (a3), W. Pessemier (a3), C. Waelkens (a3), Y. Frémat (a1), L. Dumortier (a1), A. Jorissen (a4), S. Van Eck (a4) and H. Lehmann (a5)...

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