The light curve of SN 1987 A

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Other literature type 01 Jan 1988 English Publisher:Springer Science and Business Media LLCJournal:International Astronomical Union Colloquium, volume 108, pages 438-439 (issn: 0252-9211,

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Authors: R. Schaeffer; M. Cassé; R. Mochkovitch; S. Cahen;

doi: 10.1007/bfb0034641 , 10.1017/s0252921100094318

The light curve of SN 1987 A

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Abstract

AbstractWe 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.

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Centre national de la recherche scientifique
France

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