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The Red Supergiant Progenitor of Supernova 2012aw (PTF12bvh) in Messier 95

Van Dyk, Schuyler D. and Cenko, S. Bradley and Poznanski, Dovi and Arcavi, Iair and Gal-Yam, Avishay and Filippenko, Alexei V. and Silverio, Kathryn and Stockton, Alan and Cuillandre, Jean-Charles and Marcy, Geoffrey W. and Howard, Andrew W. and Isaacson, Howard (2012) The Red Supergiant Progenitor of Supernova 2012aw (PTF12bvh) in Messier 95. Astrophysical Journal, 756 (2). Art. No. 131. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20121030-134132487

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Abstract

We report on the direct detection and characterization of the probable red supergiant (RSG) progenitor of the intermediate-luminosity Type II-Plateau (II-P) supernova (SN) 2012aw in the nearby (10.0 Mpc) spiral galaxy Messier 95 (M95; NGC 3351). We have identified the star in both Hubble Space Telescope images of the host galaxy, obtained 17-18 yr prior to the explosion, and near-infrared ground-based images, obtained 6-12 yr prior to the SN. The luminous supergiant showed evidence for substantial circumstellar dust, manifested as excess line-of-sight extinction. The effective total-to-selective ratio of extinction to the star was R'_V ≈ 4.35, which is significantly different from that of diffuse interstellar dust (i.e., R_V = 3.1), and the total extinction to the star was therefore, on average, A_V ≈ 3.1 mag. We find that the observed spectral energy distribution for the progenitor star is consistent with an effective temperature of 3600 K (spectral type M3), and that the star therefore had a bolometric magnitude of –8.29. Through comparison with recent theoretical massive-star evolutionary tracks we can infer that the RSG progenitor had an initial mass 15 ≲ M_(ini)(M_☉) < 20. Interpolating by eye between the available tracks, we surmise that the star had initial mass ~17-18 M_☉. The circumstellar dust around the progenitor must have been destroyed in the explosion, as the visual extinction to the SN is found to be low (AV = 0.24 mag with R_V = 3.1).


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/756/2/131DOIArticle
http://iopscience.iop.org/0004-637X/756/2/131PublisherArticle
ORCID:
AuthorORCID
Van Dyk, Schuyler D.0000-0001-9038-9950
Cenko, S. Bradley0000-0003-1673-970X
Arcavi, Iair0000-0001-7090-4898
Gal-Yam, Avishay0000-0002-3653-5598
Filippenko, Alexei V.0000-0003-3460-0103
Marcy, Geoffrey W.0000-0002-2909-0113
Howard, Andrew W.0000-0001-8638-0320
Isaacson, Howard0000-0002-0531-1073
Additional Information:© 2012 American Astronomical Society. Received 2012 May 27; accepted 2012 July 11; published 2012 August 22. We thank the referee for useful comments that helped improve this manuscript. This work is based in part on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute (STScI), which is operated by AURA, Inc., under NASA contract NAS5-26555. We thank Nancy Elias-Rosa for initial analysis of the HST and CFHT images, and Mark Sullivan for information about the upper limit to the SN 2012aw/PTF12bvh detection by PTF. Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA; the observatory was made possible by the generous financial support of the W. M. Keck Foundation. A.G. is supported by grants from the ISF, BSF, and GIF foundations, a Weizmann Minerva grant, and the Lord Sieff of Brimpton Fund. The research of A.V.F. and his group at UC Berkeley is funded by Gary and Cynthia Bengier, the Richard and Rhoda Goldman Fund, NSF grant AST-0908886, the TABASGO Foundation, and NASA/HST grant AR-12623 from STScI. This work was supported in part by the NSF grant PHY-1066293 and the hospitality of the Aspen Center for Physics. We dedicate this paper to the memory of our dear friend and colleague, Weidong Li, with whom two of us (A.V.F. and S.D.V.) spent many fun years identifying the progenitor stars of SNe; his tragic passing deeply saddened those who knew him.
Group:Infrared Processing and Analysis Center (IPAC), Palomar Transient Factory
Funders:
Funding AgencyGrant Number
Israel Science FoundationUNSPECIFIED
Binational Science Foundation (USA-Israel)UNSPECIFIED
German-Israeli Foundation for Research and DevelopmentUNSPECIFIED
Weizmann MinervaUNSPECIFIED
Lord Sieff of Brimpton FundUNSPECIFIED
Gary and Cynthia BengierUNSPECIFIED
Richard and Rhoda Goldman FundUNSPECIFIED
NSFAST-0908886
TABASGO FoundationUNSPECIFIED
NASAAR-12623
NSFPHY-1066293
Subject Keywords:galaxies: individual (Messier 95, NGC 3351); stars: evolution; stars: fundamental parameters; stars: late-type; supernovae: general; supernovae: individual (SN 2012aw)
Issue or Number:2
Record Number:CaltechAUTHORS:20121030-134132487
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20121030-134132487
Official Citation:The Red Supergiant Progenitor of Supernova 2012aw (PTF12bvh) in Messier 95 Schuyler D. Van Dyk et al. 2012 ApJ 756 131
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:35179
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:31 Oct 2012 18:05
Last Modified:03 Oct 2019 04:25

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