Abstract
This Letter presents wide-field optical and near-IR
(UBVRIHαK') images of the galaxy M74 that were taken
between 0.6 and 8.3 yr before the discovery of the Type Ic supernova
2002ap. We have located the position of the supernova on these images
with an accuracy of 0.3". We find no sign of a progenitor object on any
of the images. The deepest of these images is the B-band exposure, which
has a sensitivity limit corresponding to an absolute magnitude of
MB
| Original language | English |
|---|---|
| Journal | Astrophysical Journal |
| Volume | 572 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 1 Jun 2002 |
Keywords / Materials (for Non-textual outputs)
- Stars: Binaries: Close
- Galaxies: Individual: NGC Number: NGC 628
- Gamma Rays: Bursts
- Stars: Evolution
- Stars: Wolf-Rayet
- Stars: Supernovae: Individual: Alphanumeric: SN 2002ap
Fingerprint
Dive into the research topics of 'On the Progenitor of the Type Ic Supernova 2002ap'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver