Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-20T06:33:01.946Z Has data issue: false hasContentIssue false
  • English
  • Français

Relative frequencies of supernovae versus properties of spiral hosts

Published online by Cambridge University Press:  25 July 2014

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  and
J. M. Gomes
...Show all authors
A. A. Hakobyan
Affiliation:
Byurakan Astrophysical Observatory, 0213 Byurakan, Aragatzotn Province, Armenia email: [email protected]
T. A. Nazaryan
Affiliation:
Byurakan Astrophysical Observatory, 0213 Byurakan, Aragatzotn Province, Armenia email: [email protected]
V. Zh. Adibekyan
Affiliation:
Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
A. R. Petrosian
Affiliation:
Byurakan Astrophysical Observatory, 0213 Byurakan, Aragatzotn Province, Armenia email: [email protected]
L. S. Aramyan
Affiliation:
Byurakan Astrophysical Observatory, 0213 Byurakan, Aragatzotn Province, Armenia email: [email protected]
D. Kunth
Affiliation:
Institut d'Astrophysique de Paris, 98 bis Bd Arago, 75014 Paris, France
G. A. Mamon
Affiliation:
Institut d'Astrophysique de Paris, 98 bis Bd Arago, 75014 Paris, France
V. de Lapparent
Affiliation:
Institut d'Astrophysique de Paris, 98 bis Bd Arago, 75014 Paris, France
E. Bertin
Affiliation:
Institut d'Astrophysique de Paris, 98 bis Bd Arago, 75014 Paris, France
J. M. Gomes
Affiliation:
Centro de Astrofísica da Universidade do Porto, Rua das Estrelas, 4150-762 Porto, Portugal
M. Turatto
Affiliation:
INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

Keywords

supernovae: general – galaxies: spiral
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S304: Multiwavelength AGN Surveys and Studies , October 2013 , pp. 339 - 340
Copyright
Copyright © International Astronomical Union 2014 

References

Boissier, S. & Prantzos, N. 2009, A&A, 503, 137Google Scholar
Eldridge, J. J., Izzard, R. G., & Tout, C. A. 2008, MNRAS, 384, 1109CrossRefGoogle Scholar
Hakobyan, A. A., Adibekyan, V. Z., Aramyan, L. S., et al. 2012, A&A, 544, A81Google Scholar
Hakobyan, A. A., Nazaryan, T. A., Adibekyan, V. Z., et al. 2014, submittedGoogle Scholar