Adaptive optics discovery of supernova 2004ip in the nuclear regions of the luminous infrared galaxy IRAS 18293-3413

Mattila, S; Vaisanen P.; Farrah, D; Efstathiou, A; Meikle, WPS; Dahlen, T; Fransson, C; Lira, P; Lundqvist P.; Ostlin, G.; Ryder, S; Sollerman, J

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