Physics
Scientific paper
Jul 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11675m&link_type=abstract
HST Proposal ID #11675. Cycle 17
Physics
Scientific paper
Recent studies have used high spatial resolution HST observations of SN sites to identify the progenitors of core-collapse SNe on pre-explosion images. These studies have set constraints about the nature of massive stars and their evolution just prior to their explosion as SNe. Now, at late-times when the SNe have faded sufficiently, it is possible to return to the sites of these core-collapse SNe to search for clues about the nature of their progenitors. We request time to conduct deep, late-time, high-resolution imaging with ACS/HRC of the sites of six core-collapse SNe. In this program we aim to: 1} confirm our identifications, that were made with HST pre-explosion images, of the red supergiant progenitors of four Type IIP SNe {1999ev, 2003gd, 2004A and 2005cs}, by observing if the objects identified as the progenitors are now missing; 2} place precise constraints on the progenitor of the Type Ic SN 2007gr by studying its host cluster; and 3} confirm our identification of an LBV-like outburst of an unstable WR star as belonging to the progenitor of a Type Ib-n core-collapse SN {2006jc}, using broad and narrow-band imaging to search for emission line stars in its locality. The deep imaging will also allow to probe the stellar populations in the immediate vicinities of these SNe, that were previously obscured by the progenitors and the bright SNe. HST provides the unique combination of high-resolution optical imaging at very faint magnitudes that will facilitate this study.;
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