Adaptive optics discovery of supernova 2004ip in the nuclear regions of the luminous infrared galaxy IRAS 18293-3413
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. © 2007. The American Astronomical Society. All rights reserved.
Más información
Título según WOS: | Adaptive optics discovery of supernova 2004ip in the nuclear regions of the luminous infrared galaxy IRAS 18293-3413 |
Título según SCOPUS: | Adaptive optics discovery of supernova 2004ip in the nuclear regions of the luminous infrared galaxy IRAS 18293-3413 |
Título de la Revista: | ASTROPHYSICAL JOURNAL |
Volumen: | 659 |
Número: | 1 |
Editorial: | IOP PUBLISHING LTD |
Fecha de publicación: | 2007 |
Página de inicio: | L9 |
Página final: | L12 |
Idioma: | English |
URL: | http://stacks.iop.org/1538-4357/659/i=1/a=L9 |
DOI: |
10.1086/516821 |
Notas: | ISI, SCOPUS |