Low-Mass Neutron Stars as Anomalous Pulsars

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dc.creatorSeward, Frederick D.
dc.date2001-12-03
dc.date.accessioned2026-07-07T02:01:39Z
dc.date.available2026-07-07T02:01:39Z
dc.descriptionA 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.
dc.description4 pages, 3 figures, to appear in "Neutron Stars in Supernova Remnants" (ASP Conference Proceedings), eds P.O. Slane and B.M. Gaensler
dc.identifierhttps://arxiv.org/abs/astro-ph/0112047
dc.identifierhttp://arxiv.org/abs/astro-ph/0112047
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3827
dc.subjectAstrophysics
dc.titleLow-Mass Neutron Stars as Anomalous Pulsars
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