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The Rate of Supernovae in Normal Galaxies

Published online by Cambridge University Press:  25 May 2016

Enrico Cappellaro
Enrico Cappellaro*
Affiliation:
Osservatorio Astronomico di Padova, vicolo dell'Osservatorio 5, Padova, I-35122, Italy

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The rate of supernovae (SNe) is a key number linking stellar evolution with galaxy evolution models. Stellar evolution theories predict life times, fates and nucleosysntesis yields of individual stars which are used to predicted the galaxy chemical evolution once the star formation history in the galaxy is known. Constraints to the models are the present chemical content of galaxies but also the present observed SN rate (Arimoto & Yoshi, 1987; Ferrini & Poggianti, 1993; Matteucci, 1994; Renzini et al., 1993; Bressan et al., 1994; Elbaz et al., 1995).

Type
Elliptical Galaxies
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 81 - 84
Copyright
Copyright © Kluwer 1996 

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