Mixing due to Rayleigh-Taylor instabilities in SN 1987A.

Details Mixing due to Rayleigh-Taylor instabilities in SN 1987A. Mixing due to Rayleigh-Taylor instabilities in SN 1987A.

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nuas.conf..103m&link_type=abstract

"Proceedings of the 5th Workshop on Nuclear

Physics

Supernova 1987A In Lmc, Supernovae: Shock Waves

Scientific paper

The early discovery of soft and hard X-rays as well as of γ-ray line emission from supernova 1987A indicates that radioactive 56Co has been mixed from the deep interior of the exploding star into the hydrogen-rich envelope. This paper reports numerical simulations of the mixing process by modeling the supernova explosion using a 3-d explicit Eulerian hydrodynamic code.

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