Low-Mass Neutron Stars as Anomalous Pulsars

Details Low-Mass Neutron Stars as Anomalous Pulsars Low-Mass Neutron Stars as Anomalous Pulsars

2001-12-03

arxiv.org/abs/astro-ph/0112047v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures, to appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P.O. Slane and B.M. G

Scientific paper

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.

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