Evidence of a massive black hole companion in the massive eclipsing binary V Puppis

Up to now, most stellar-mass black holes have been discovered in X-ray-emitting binaries, in which the black holes are formed through a common-envelope evolution. Here we give evidence for the presence of a massive black hole candidate as a tertiary companion in the massive eclipsing binary V Puppis...

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Detalles Bibliográficos
Autores principales:	Qian, S. B., Liao, W. P., Fernández Lajús, Eduardo
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2008
Materias:	Ciencias Astronómicas Binaries: Close Binaries: Eclipsing Black hole physics Stars: Evolution Stars: Individual (V Puppis)
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/83468
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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