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RCW 103 — revisiting a cooling neutron star
Authors:Jeremy S. Heyl,&   Lars Hernquist
Affiliation:Lick Observatory, University of California, Santa Cruz, California 95064, USA
Abstract:
Recent observations of the compact source embedded within the supernova remnant RCW 103 rekindle interest in the origin of this object's emission. We contrast several models in which neutron-star cooling powers RCW 103. Specifically, either the presence of an accreted envelope or a sufficiently intense magnetic field can account for the X-ray emission from this object.
Keywords:radiative transfer    stars: magnetic fields    stars: neutron    X-rays: stars
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