Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, A29B(11), p. 257-258, 2015

DOI: 10.1017/s1743921316005238

Links

Tools

Export citation

Search in Google Scholar

Stripped-envelope supernova rates and host-galaxy properties

Journal article published in 2015 by Or Graur ORCID, F. B. Bianco, M. Modjaz, D. Maoz, I. Shivvers, A. V. Filippenko, W. Li
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Upload
Green circle
Postprint: archiving allowed
Upload
Red circle
Published version: archiving forbidden
Policy details
Data provided by SHERPA/RoMEO

Abstract

AbstractThe progenitors of stripped-envelope supernovae (SNe Ibc) remain to be conclsuively identified, but correlations between SN rates and host-galaxy properties can constrain progenitor models. Here, we present one result from a re-analysis of the rates from the Lick Observatory Supernova Search. Galaxies with stellar masses ≲1010 M⊙ are less efficient at producing SNe Ibc than more massive galaxies. Any progenitor scenario must seek to explain this new observation.

Beta version