Relative frequencies of supernovae versus properties of spiral hosts

A. A. Hakobyan, T. A. Nazaryan, V. Zh. Adibekyan, A. R. Petrosian, L. S. Aramyan, D. Kunth, G. A. Mamon, V. de Lapparent, E. Bertin, J. M. Gomes, M. Turatto

Abstract
In this work, we present an analysis of SNe number ratios in spiral galaxies with different morphological subtypes, luminosities, sSFR, and metallicities, to provide important information about the physical properties of the progenitor populations.

Multiwavelength AGN Surveys and Studies
(Eds.) Z. Kne¸ević, A. Lemaitre

Cambridge University Press
Vol. 9, Page 339
2014

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