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The log N-log S Distributions of Accreting and Cooling Isolated Neutron Stars

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Published 2000 November 1 © 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation S. B. Popov et al 2000 ApJ 544 L53 DOI 10.1086/317295

1538-4357/544/1/L53

Abstract

We model populations of isolated neutron stars in the Galaxy following their orbital and magnetorotational evolution. It is shown that accretors become more abundant than coolers at fluxes below ~10-13 ergs cm-2 s-1, and one can predict that about one accreting neutron star per square degree should be observed at the Chandra and Newton flux limits of ~10-16 ergs cm-2 s-1. The soft ROSAT sources associated with isolated neutron stars can be relatively young cooling objects only if the neutron star birthrate in the solar vicinity during the last ~106 yr is higher than that inferred from radio pulsar observations.

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10.1086/317295