Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...408l..25f&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 408, no. 1, p. L25-L28.
Astronomy and Astrophysics
Astrophysics
54
Light Curve, Nuclear Fusion, Supernova 1987A, Abundance, Bolometers, Emission Spectra, Neutron Stars
Scientific paper
After about 800 days, time-dependent effects due to long recombination and cooling times lead to a frozen-in structure of the ejecta of SN 1987A. The result is a higher bolometric luminosity, compared to models where the emitted luminosity is equal to the instantaneous energy input. Good agreement with the observed light curve of SN 1987A is obtained with an initial (Ni-57)/(Ni-56) ratio 2 times the solar (Fe-57)/(Fe-56) ratio, while steady state models require a factor of 2 more. Consistency with both the Co-57 mass from IR line observations, X-ray, and gamma-ray observations, and from models of the nucleosynthesis can thus be obtained.
Fransson Claes
Kozma Cecilia
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