Relative frequencies of supernovae versus properties of spiral hosts
arXiv:1312.5896 · doi:10.1017/S1743921314004220
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.
2 pages, 1 figure