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GALEX Detection of Shock Breakout in Type IIP Supernova PS1-13arp: Implications for the Progenitor Star Wind

Gezari, S. and Martin, D. C. (2015) GALEX Detection of Shock Breakout in Type IIP Supernova PS1-13arp: Implications for the Progenitor Star Wind. Astrophysical Journal, 804 (1). Art. No. 28. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20150608-080924860

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Abstract

We present the GALEX detection of a UV burst at the time of explosion of an optically normal supernova (SN) IIP (PS1-13arp) from the Pan-STARRS1 survey at z = 0.1665. The temperature and luminosity of the UV burst match the theoretical predictions for shock breakout in a red supergiant (RSG), but with a duration a factor of ~50 longer than expected. We compare the NUV light curve of PS1-13arp to previous GALEX detections of SNe IIP and find clear distinctions that indicate that the UV emission is powered by shock breakout, and not by the subsequent cooling envelope emission previously detected in these systems. We interpret the ~1 day duration of the UV signal with a shock breakout in the wind of an RSG with a pre-explosion mass-loss rate of ~ 10^(-3) M_☉ yr^(−1). This mass-loss rate is enough to prolong the duration of the shock breakout signal, but not enough to produce an excess in the optical plateau light curve or narrow emission lines powered by circumstellar interaction. This detection of non-standard, potentially episodic high mass loss in an RSG SN progenitor has favorable consequences for the prospects of future wide-field UV surveys to detect shock breakout directly in these systems, and provide a sensitive probe of the pre-explosion conditions of SN progenitors.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/804/1/28DOIArticle
http://iopscience.iop.org/0004-637X/804/1/28/PublisherArticle
http://arxiv.org/abs/1502.06964arXivDiscussion Paper
Additional Information:© 2015 American Astronomical Society. Received 2015 January 26; accepted 2015 February 23; published 2015 April 27. S.G. thanks the Gemini Deputy Director for approving a change of program for the TOO program GN-2013A-Q-32 to observe PS1-13arp. The Pan-STARRS1 Surveys (PS1) have been made possible through contributions of the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg, and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, Queen’s University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation under grant No. AST-1238877, the University of Maryland, and Eotvos Lorand University (ELTE).
Group:Space Astrophysics Laboratory
Funders:
Funding AgencyGrant Number
NASANNX08AR22G
NSFAST-1238877
Subject Keywords:supernovae: individual (PS1-13arp); surveys; ultraviolet: general
Record Number:CaltechAUTHORS:20150608-080924860
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20150608-080924860
Official Citation:GALEX Detection of Shock Breakout in Type IIP Supernova PS1-13arp: Implications for the Progenitor Star Wind S. Gezari et al. 2015 ApJ 804 28
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:58068
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:08 Jun 2015 15:35
Last Modified:26 Aug 2016 22:22

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