The discovery of binary white dwarfs that will merge within 500 Myr

We present radial velocity observations of four extremely low-mass (0.2 M⊙) white dwarfs (WDs). All four stars show peak-to-peak radial velocity variations of 540-710kms-1 with 1.0-5.9hr periods. The optical photometry rules out main-sequence companions. In addition, no millisecond pulsar companions...

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Autores principales: Kilic, M., Brown, W.R., Allende Prieto, C., Kenyon, S.J., Panei, Jorge Alejandro
Formato: Articulo
Lenguaje:Inglés
Publicado: 2010
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/82486
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