Statistics
Scientific paper
Jul 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84..985o&link_type=abstract
Astronomical Journal, vol. 84, July 1979, p. 985-992.
Statistics
120
Galactic Structure, Stellar Evolution, Supernovae, Distance, Elliptical Galaxies, Protostars, Spiral Galaxies, Stellar Luminosity
Scientific paper
Statistics for a sample of 178 supernovae in external galaxies are presented which show convincingly that at least most Type I supernovae (SN I), viz., those in spiral and irregular galaxies, are associated with a young stellar population. Relative SN rates in galaxies of different types are discussed which establish an association between SN I and newly formed stars, at least in spirals and irregulars, and SN rates in spirals are derived as a function of color, confirming this association. Problems of associating SN I in elliptical galaxies with ongoing star formation are also considered. It is concluded that SN I have fairly short-lived precursors, with lifetimes between a few tens of millions of years and a few hundred million years.
Oemler Augustus Jr.
Tinsley Beatrice M.
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