Abstract
The pre-explosion observations of the Type II-P supernovae 2006my, 2006ov and 2004et are re-analysed. In the cases of supernovae 2006my and 2006ov we argue that the published candidate progenitors are not coincident with their respective supernova sites in pre-explosion Hubble Space Telescope observations. We therefore derive upper luminosity and mass limits for the unseen progenitors of both these supernovae, assuming they are red supergiants: 2006my (log L/L-circle dot = 4.51; m
| Original language | English |
|---|---|
| Pages (from-to) | 2767-2786 |
| Number of pages | 20 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 410 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - Feb 2011 |
ASJC Scopus subject areas
- Space and Planetary Science
- Astronomy and Astrophysics