On the frequency of supernova flares in SC galaxies

Mathematics – Probability

Scientific paper

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Spiral Galaxies, Stellar Flares, Supernovae, Flare Stars, Galactic Structure, Luminosity, Probability Theory

Scientific paper

The mean frequency of supernova explosions in Sc galaxies is determined by a method used to calculate the mean frequency of the flares of flare stars in star aggregates. The mean time interval between two successive supernova explosions in one Sc galaxy brighter than 12.0 magnitudes is 48 years. It has not been possible to find clear dependence of the frequency of supernova explosions on the luminosity of the parent galaxy for the considered group of galaxies.

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