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Accretion onto Magnetized Neutron Stars

Published online by Cambridge University Press:  25 April 2016

J. G. Kirk
J. G. Kirk*
Affiliation:
Department of Theorectical Physics, University of Sydney, Sydney N.S.W. 2006, Australia
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Extract

Magnetic fields of about 1012 G have now been measured in several astrophysical objects (Trümper etal. 1978, Wheaton et al. 1979, Mazets et al. 1981). In the case of pulsating X-ray sources, the presence of a companion star indicates that accretion is probably the energy source for the X-rays.

Type
Invited Papers
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 446 - 456
Copyright
Copyright © Astronomical Society of Australia 1984

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