Supernova 1987A and the emergence of the hot neutron star - A semianalytic approach

Details Supernova 1987A and the emergence of the hot neutron star - A semianalytic approach Supernova 1987A and the emergence of the hot neutron star - A semianalytic approach

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...337..814c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 337, Feb. 15, 1989, p. 814-822.

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Computational Astrophysics, Hot Stars, Neutron Stars, Stellar Evolution, Supernova 1987A, Density Distribution, Gamma Rays, Stellar Envelopes, Stellar Interiors, Stellar Luminosity, X Ray Astronomy

Scientific paper

Supernova 1987A is modeled as a Sedov blast wave in a star with a power-law density distribution. The evolution of the optical depth for absorption and scattering is treated as a function of frequency. The general question of when a source of frequency and luminosity first becomes visible at the center of the remnant is addressed. The possibility of detecting thermal X-rays from the hot neutron star surface and gamma rays from a pulsar is addressed.

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