Yayınlanmış 1 Ocak 2003 | Sürüm v1
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Do young neutron stars which show themselves as AXPs and SGRs accrete?

Açıklama

We examined the fall-back disk models, and in general accretion, proposed to explain the properties of AXPs and SGRs. We checked the possibility of some gas remaining around the neutron star after a supernova explosion. We also compared AXPs and SGRs with the X-ray pulsars in X-ray binaries. We conclude that the existing models of accretion from a fall-back disk are insufficient to explain the nature of AXPs and SGRs.

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