Neutron star accretion in a supernova

Details Neutron star accretion in a supernova Neutron star accretion in a supernova

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...346..847c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 346, Nov. 15, 1989, p. 847-859.

Astronomy and Astrophysics

Astronomy

196

Accretion Disks, Neutron Stars, Supernova 1987A, Black Holes (Astronomy), Shock Waves, Stellar Magnetic Fields, Stellar Mass Accretion, Stellar Rotation

Scientific paper

An estimate can be made of the effect of a central mass on an explosion through the study of self-similar blast waves in a medium having an inverse-square-of-r density profile, as is approximately the case in the inner core of the progenitor of SN 1987A; its parameters are such that the nucleon density is substantially constant within the shock front. In SN explosions with a massive envelopes, the core material is decelerated by its interaction with the envelope, and a reverse shock wave propagates back to the center.

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