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The Magnetic Fields and Original Spins of Binary and Runaway Pulsars

Published online by Cambridge University Press:  14 August 2015

F. K. Lamb
F. K. Lamb*
Affiliation:
Departments of Physics and Astronomy, University of Illinois at Urbana-Champaign

Extract

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Pulsing X-ray sources are believed to be the progenitors of binary and runaway pulsars. Thus, their observed properties and predicted fates furnish information about the initial properties and evolution of these pulsars. Evidence is discussed which suggests that many binary and runaway pulsars are born with periods ~ seconds and dipole magnetic fields ~ 1011 – 1013 G, and that the turnoff of at least some is not due to decay of their dipole magnetic fields.

Type
VIII. Neutron Stars in Binary Systems
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 357 - 360
Copyright
Copyright © Reidel 1981 

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