Supernovae Light Curves : Clues to the Progenitor and Explosions, using Flux-Limited Diffusion

Details Supernovae Light Curves : Clues to the Progenitor and Explosions, using Flux-Limited Diffusion Supernovae Light Curves : Clues to the Progenitor and Explosions, using Flux-Limited Diffusion

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...181.7606y&link_type=abstract

American Astronomical Society, 181st AAS Meeting, #76.06; Bulletin of the American Astronomical Society, Vol. 24, p.1244

Astronomy and Astrophysics

Astrophysics

Scientific paper

Numerical light curve calculations are compared to observations of the type Ib SN 1984L and the type II-L SN 1970G. Spectroscopic and photometric observations of SN 1984L lead to contradictory conclusions. At early times a high mass/low energy is suggested while at late times a low mass/high energy is implied. Results show that an ejected mass of 50 M_sun of He with an energy of 2.4x10(52) fits the light curve, but these parameters lead to an astrophysical anomally.

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