{ "id": "1106.2565", "version": "v1", "published": "2011-06-13T21:18:28.000Z", "updated": "2011-06-13T21:18:28.000Z", "title": "The Yellow Supergiant Progenitor of the Type II Supernova 2011dh in M51", "authors": [ "J. R. Maund", "M. Fraser", "M. Ergon", "A. Pastorello", "S. J. Smartt", "J. Sollerman", "S. Benetti", "M. -T. Botticella", "F. Bufano", "I. J. Danziger", "R. Kotak", "L. Magill", "A. W. Stephens", "S. Valenti" ], "comment": "Submitted to ApJ Letters - 6 pages, 5 figures", "categories": [ "astro-ph.SR" ], "abstract": "We present the detection of the progenitor of the Type II SN 2011dh in archival pre-explosion Hubble Space Telescope images. Using post-explosion Adaptive Optics imaging with Gemini NIRI+ALTAIR, the position of the SN in the pre-explosion images was determined to within 23mas. The progenitor object was found to be consistent with a F8 supergiant star (log L/L_{\\odot}=4.92+/-0.20 and T_{eff}=6000+/-280K). Through comparison with stellar evolution tracks, this corresponds to a single star at the end of core C-burning with an initial mass of M_{ZAMS}=13+/-3M_{\\odot}. The possibility of the progenitor source being a cluster is rejected, on the basis of: 1) the source is not spatially extended; 2) the absence of excess H\\alpha\\, emission; and 3) the poor fit to synthetic cluster SEDs. It is unclear if a binary companion is contributing to the observed SED, although given the excellent correspondence of the observed photometry to a single star SED we suggest the companion does not contribute significantly. Early photometric and spectroscopic observations show fast evolution similar to the transitional Type IIb SN 2008ax, and suggest that a large amount of the progenitor's hydrogen envelope was removed before explosion.", "revisions": [ { "version": "v1", "updated": "2011-06-13T21:18:28.000Z" } ], "analyses": { "keywords": [ "yellow supergiant progenitor", "supernova 2011dh", "hubble space telescope images", "pre-explosion hubble space telescope", "transitional type iib sn 2008ax" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/739/2/L37", "journal": "The Astrophysical Journal", "year": 2011, "month": "Oct", "volume": 739, "number": 2 }, "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable", "inspire": 913638, "adsabs": "2011ApJ...739L..37M" } } }