Relative frequencies of supernovae versus properties of spiral hosts

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.

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Bibliographic Details
Published inProceedings of the International Astronomical Union Vol. 9; no. S304; pp. 339 - 340
Main Authors Hakobyan, A. A., Nazaryan, T. A., Adibekyan, V. Zh, Petrosian, A. R., Aramyan, L. S., Kunth, D., Mamon, G. A., de Lapparent, V., Bertin, E., Gomes, J. M., Turatto, M.
Format Journal Article
LanguageEnglish
Published Cambridge, UK Cambridge University Press 01.10.2013
Subjects
Contributed Papers
Frequencies
Stars & galaxies
Supernovae
supernovae: general – galaxies: spiral
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Summary: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.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921314004220