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Intermittent stellar wind accretion in Pop. I binary systems containing an X-ray pulsar

✍ Scribed by L. Stella; N. E. White; R. Rosner


Publisher
Springer Netherlands
Year
1985
Tongue
English
Weight
486 KB
Volume
40
Category
Article
ISSN
0038-6308

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✦ Synopsis


We review the long term variability properties of accretion powered X-ray pulsars in massive Pop. I binary systems and discuss how their characteristics, in particular the large dynamic range in luminosity of the transient pulsars, can be understood in terms of the interaction of the accreting material with the neutron star magnetosphere. We point out that the X-ray pulsar transient activity in general can be due to the transition between direct wind accretion and a regime in which the centrifugal drag exerted by the pulsar magnetosphere inhibits accretion onto the neutron star surface.