Supernova theory and supernova 1987A

Details Supernova theory and supernova 1987A Supernova theory and supernova 1987A

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987apj...319..136a&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 319, Aug. 1, 1987, p. 136-142.

Astronomy and Astrophysics

Astrophysics

126

Stellar Interiors, Stellar Models, Stellar Spectrophotometry, Supernova 1987A, Abundance, Neutrinos, Stellar Evolution, Stellar Mass

Scientific paper

The implications of Supernova 1987A are examined and compared with theoretical expectations. The relatively low luminosity follows from the progenitor having lower than solar abundances. The explosion energy is (1.0 - 2.0)×1051ergs for a 15 M_sun; star. The neutrino signal is strikingly that expected from recent models of the core collapse process with advective overturn.

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