VLT Detection of a Red Supergiant Progenitor of the Type II-P Supernova 2008bk

We report the identification of a source coincident with the position of the nearby Type II-P supernova (SN) 2008bk in high-quality optical and near- infrared preexplosion images from the ESO Very Large Telescope (VLT). The SN position in the optical and near-infrared preexplosion images is identifi...

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Published inThe Astrophysical journal Vol. 688; no. 2; pp. L91 - L94
Main Authors Mattila, S, Smartt, S. J, Eldridge, J. J, Maund, J. R, Crockett, R. M, Danziger, I. J
Format Journal Article
LanguageEnglish
Published Bristol IOP Publishing 01.12.2008
IOP
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ISSN1538-4357
0004-637X
1538-4357
DOI10.1086/595587

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Summary:We report the identification of a source coincident with the position of the nearby Type II-P supernova (SN) 2008bk in high-quality optical and near- infrared preexplosion images from the ESO Very Large Telescope (VLT). The SN position in the optical and near-infrared preexplosion images is identified to within about +/-70 and +/-40 mas, respectively, using postexplosion [image] -band images obtained with the NAOS CONICA adaptive optics system on the VLT. The preexplosion source detected in four different bands is precisely coincident with SN 2008bk and is consistent with being dominated by a single point source. We determine the nature of the point source using the STARS stellar evolutionary models and find that its colors and luminosity are consistent with the source being a red supergiant progenitor of SN 2008bk with an initial mass of 8.5 +/- 1.0 M[image].
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ISSN:1538-4357
0004-637X
1538-4357
DOI:10.1086/595587