Abstract
The 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.
| Original language | English |
|---|---|
| Pages (from-to) | 257-258 |
| Number of pages | 2 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 11 |
| Issue number | A29B |
| DOIs | |
| State | Published - 2015 |
Keywords
- galaxies: fundamental parameters
- supernovae: general
- surveys