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Paper: Low-Mass Neutron Stars as Anomalous Pulsars
Volume: 271, Neutron Stars in Supernova Remnants
Page: 270
Authors: Seward, F. D.
Abstract: 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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