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Light curve fittings of active galactic nuclei using supernova explosions
Authors:Itziar Aretxaga  Angeles I Díaz  Roberto Terlevich  Elena Terlevich
Institution:(1) Depto. de Física Teórica, Universidad Autónoma de Madrid, Cantoblanco, Madrid, Spain;(2) Royal Greenwich Observatory, Herstmonceux, U.K.
Abstract:In the starburst-warmers scenario, we have used a supernova (SN) explosion model to construct theoretical light curves for active galactic nuclei (AGN). The ionizing flux, in this model, should show variability according to the SN rate in the galaxy.Paper presented at the 11th European Regional Astronomical Meetings of the IAU on lsquoNew Windows to the Universersquo, held 3–8 July, 1989, Tenerife, Canary Islands, Spain.
Keywords:
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