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Bringing the Visible Universe into Focus with Robo-AO
Published on: February 12, 2013
Tugboat model for OB binaries, X-ray stars and pulsars
1Department of Physics and Astronomy, University of Massachusetts, Amherst, MA 01003, USA.
Nature
|May 12, 1977
Abstract:
An examination of the kinematical properties of binary OB stars, binary X-ray sources and pulsars suggests an evolutionary sequence linking an apparent low-velocity class of pulsars to the binary nature of their extreme Population I progenitors.
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