Abstract
We report a supernova discovery in Ks-band images from the NAOS CONICA adaptive optics (AO) system on the ESO Very Large Telescope. The images were obtained as part of a near-infrared search for highly obscured supernovae in the nuclear regions of luminous and ultraluminous infrared galaxies. SN 2004ip is located within a circumnuclear starburst at 1.4″ (or 500 pc) projected distance from the K-band nucleus of the luminous infrared galaxy IRAS 18293 -3413. The supernova luminosity and light curve are consistent with a core-collapse event suffering from a host galaxy extinction of up to about 40 mag in the V band, which is as expected for a circumnuclear starburst environment. This is the first supernova to be discovered making use of AO correction and demonstrates the potential of the current 8 m-class telescopes equipped with AO in discovering supernovae from the innermost nuclear regions of luminous and ultraluminous infrared galaxies.
| Original language | English |
|---|---|
| Pages (from-to) | L9-L12 |
| Number of pages | 4 |
| Journal | The Astrophysical Journal |
| Volume | 659 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - 10 Apr 2007 |
| Externally published | Yes |
Keywords
- Galaxies: individual (IRAS 18293-3413)
- Galaxies: starburst
- Infrared: galaxies
- Instrumentation: adaptive optics
- Supernovae: general
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