Thermal radiation of neutron stars

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 1987 English Publisher:Springer Science and Business Media LLCJournal:Astrophysics, volume 26, pages 155-161 (issn: 0571-7132, eissn: 1573-8191,

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Authors: G. G. Arutyunyan; V. V. Papoyan; G. S. Saakyan;

doi: 10.1007/bf01005553

Thermal radiation of neutron stars

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Abstract

The parameters that characterize the thermal evolution of neutron stars whose hadronic matter contains a ..pi../sup -/ meson component are found. It is shown that the surface temperature T/sub R/ of typical neutron stars varies in the range 10/sup 5/ less than or equal to T/sub R/ less than or equal to 10/sup 6/. For T/sub R/ > 10/sup 6/, their cooling is basically due to neutrino losses. For stars with lifetime 10/sup 3/-10/sup 6/ year, the photon luminosity is of order 10/sup 29/-10/sup 33/ ergsec

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