Abstract
We present images taken with the Gemini Multi-Object Spectrograph on Gemini-South, in excellent (<0.5 arcsec) seeing, of supernova (SN) 2001ig in NGC 7424, ~1000 d after explosion. A point source seen at the site of the SN is shown to have colours inconsistent with being an H II region or a SN 1993J-like remnant, but can be matched to a late-B through late-F supergiant with AV < 1. We believe this object is the massive binary companion responsible for periodic modulation in mass-loss material around the Wolf-Rayet progenitor which gave rise to significant structure in the SN radio light curve.
| Original language | English |
|---|---|
| Pages (from-to) | L32-L36 |
| Number of pages | 5 |
| Journal | Monthly Notices of the Royal Astronomical Society: Letters |
| Volume | 369 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 1 Jun 2006 |
| Externally published | Yes |
Keywords
- Binaries: general
- Galaxies: individual: NGC 7424
- Stars: evolution
- Supernovae: general
- Supernovae: individual: SN 2001ig