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07 February 2025
 
  » arxiv » astro-ph/0112047

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Low-Mass Neutron Stars as Anomalous Pulsars
Frederick D. Seward ;
Date 3 Dec 2001
Subject astro-ph
AbstractA 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.
Source arXiv, astro-ph/0112047
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