Constraints on neutron star models of gamma-burst sources from the Einstein Observatory

Details Constraints on neutron star models of gamma-burst sources from the Einstein Observatory Constraints on neutron star models of gamma-burst sources from the Einstein Observatory

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...301..641p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 301, Feb. 15, 1986, p. 641-649.

Astronomy and Astrophysics

Astrophysics

43

Gamma Ray Bursts, Neutron Stars, Stellar Mass Accretion, Stellar Radiation, X Ray Sources, Heao 2, Stellar Models, Stellar Temperature

Scientific paper

Six Einstein observations of five gamma-ray burst sources are presented and discussed. With one possible exception, no point source was detected in any of the observations. The data are interpreted in the framework of neutron star models for gamma bursters. Upper limits are derived for the surface temperatures of the neutron stars assumed to be responsible for the bursts. It is shown that the lack of soft X-ray emission may impose stringent constraints on accretion rates onto neutron stars.

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