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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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