The statistical investigation of type Ib/c and II supernovae and their host galaxies

Details The statistical investigation of type Ib/c and II supernovae and their host galaxies The statistical investigation of type Ib/c and II supernovae and their host galaxies

2008-04-03

arxiv.org/abs/0804.0540v1

Astrophysics.51:69-76,2008

Astronomy and Astrophysics

Astrophysics

8 pages, 2 figures

Scientific paper

10.1007/s10511-008-0008-3

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 R(SN)/R(25) 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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