A Be-type star with a black-hole companion

Author:

Casares J.,Negueruela I.,Ribó M.,Ribas I.,Paredes J. M.,Herrero A.,Simón-Díaz S.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Reference54 articles.

1. Raguzova, N. V. & Lipunov, V. M. The evolutionary evidence for Be/black hole binaries. Astron. Astrophys. 349, 505–510 (1999)

2. Zhang, F., Li, X.-D. & Wang, Z.-R. Where are the Be/black hole binaries? Astrophys. J. 603, 663–668 (2004)

3. Belczynski, K. & Ziolkówski, J. On the apparent lack of Be X-ray binaries with black holes. Astrophys. J. 707, 870–877 (2009)

4. Ziólkowski, J. & Belczynski, K. On the apparent lack of Be X-ray binaries with black holes in the Galaxy and in the Magellanic Clouds. IAU Symp. 275, 329–330 (2011)

5. Casares, J. et al. On the binary nature of the γ-ray sources AGL J2241+4454 ( = MWC 656) and HESS J0632+057 ( = MWC 148). Mon. Not. R. Astron. Soc. 421, 1103–1112 (2012)

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