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The Light Curve of SN 1987 A
Published online by Cambridge University Press: 12 April 2016
Abstract
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We use a semi–analytical model of supernova light curves that extends Arnett’s scheme [1,2] to include the effect of recombination of hydrogen, helium and heavy elements in the expanding ejecta. Introducing in the model the physical parameters of Sanduleak −69 202, the salient characteristics of the light curve of SN 1987 A are reasonably reproduced over 100 days.
- Type
- Part III. Chemical and Dynamical Structures of Exploding Stars
- Information
- Copyright
- Copyright © Springer-Verlag 1988
References
[3]
Woosley, S.E.: 1987, in 16th Advanced Course of Saas-Fee, ed. Hauck, B., Maeder, A., Meynet, G., p. 127Google Scholar
[7]
Dopita, M.A., Achilleos, N., Dawe, J.A., Flynn, C., Meatheringham, S.J.: 1987, to be published in Proc. Astron. Soc. Austr.Google Scholar
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