Low-Mass Neutron Stars as Anomalous Pulsars

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A neutron star with mass close to the lower limit might be a reasonable model for some anomalous pulsars. Emission is thermal. X-ray luminosity is high. Spatial velocity can be high. Since the radius is predicted to be large, the magnetic field calculated for spin-down is lower than that required by the magnetar model.
4 pages, 3 figures, to appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P.O. Slane and B.M. Gaensler

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/3827

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0112047
 http://arxiv.org/abs/astro-ph/0112047

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arXiv