Abstract
This is a statistical study of the properties of type Ib/c and II supernovae and of the integral parameters of their spiral host galaxies. The methods of one-dimensional and multivariate statistics were applied to the data sample. It was found that the Ib/c supernovae are more concentrated radially toward the centers of the galaxies than those of type II. The distributions of the radial distances RSN/R25 for the type Ib/c and II supernovae in active galaxies are more concentrated toward the center than in normal galaxies. This effect is stronger for type Ib/c than for type II supernovae.
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Translated from Astrofizika, Vol. 51, No. 1, pp. 89–98 (February 2008).
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Hakobyan, A.A. The statistical investigation of type Ib/c and II supernovae and their host galaxies. Astrophysics 51, 69–76 (2008). https://doi.org/10.1007/s10511-008-0008-3
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DOI: https://doi.org/10.1007/s10511-008-0008-3