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Evidence for a Compact Wolf-Rayet Progenitor for the Type Ic Supernova PTF 10vgv

Corsi, A. and Ofek, E. O. and Gal-Yam, A. and Frail, D. A. and Poznanski, D. and Mazzali, P. A. and Kulkarni, S. R. and Kasliwal, M. M. and Arcavi, I. and Ben-Ami, S. and Cenko, S. B. and Filippenko, A. V. and Fox, D. B. and Horesh, A. and Howell, J. L. and Kleiser, I. K. W. and Nakar, E. and Rabinak, I. and Sari, R. and Silverman, J. M. and Xu, D. and Bloom, J. S. and Law, N. M. and Nugent, P. E. and Quimby, R. M. (2012) Evidence for a Compact Wolf-Rayet Progenitor for the Type Ic Supernova PTF 10vgv. Astrophysical Journal Letters, 747 (1). Art. No. L5. ISSN 2041-8205. doi:10.1088/2041-8205/747/1/L5. https://resolver.caltech.edu/CaltechAUTHORS:20120402-091946766

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Abstract

We present the discovery of PTF 10vgv, a Type Ic supernova (SN) detected by the Palomar Transient Factory, using the Palomar 48 inch telescope (P48). R-band observations of the PTF 10vgv field with P48 probe the SN emission from its very early phases (about two weeks before R-band maximum) and set limits on its flux in the week prior to the discovery. Our sensitive upper limits and early detections constrain the post-shock-breakout luminosity of this event. Via comparison to numerical (analytical) models, we derive an upper-limit of R ≾ 4.5 R_☉ (R ≾ 1 R_☉) on the radius of the progenitor star, a direct indication in favor of a compact Wolf-Rayet star. Applying a similar analysis to the historical observations of SN 1994I yields R ≾ 1/4 R_☉ for the progenitor radius of this SN.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/2041-8205/747/1/L5DOIArticle
http://iopscience.iop.org/2041-8205/747/1/L5/PublisherArticle
ORCID:
AuthorORCID
Corsi, A.0000-0001-8104-3536
Ofek, E. O.0000-0002-6786-8774
Gal-Yam, A.0000-0002-3653-5598
Mazzali, P. A.0000-0001-6876-8284
Kulkarni, S. R.0000-0001-5390-8563
Kasliwal, M. M.0000-0002-5619-4938
Arcavi, I.0000-0001-7090-4898
Ben-Ami, S.0000-0001-6760-3074
Cenko, S. B.0000-0003-1673-970X
Filippenko, A. V.0000-0003-3460-0103
Fox, D. B.0000-0002-3714-672X
Horesh, A.0000-0002-5936-1156
Nakar, E.0000-0002-4534-7089
Sari, R.0000-0002-1084-3656
Silverman, J. M.0000-0003-3325-3365
Bloom, J. S.0000-0002-7777-216X
Law, N. M.0000-0001-9380-6457
Nugent, P. E.0000-0002-3389-0586
Quimby, R. M.0000-0001-9171-5236
Additional Information:© 2012 American Astronomical Society. Received 2011 October 25; accepted 2012 January 4; published 2012 February 8. We thank Boaz Katz and Eli Waxman for useful comments. PTF is a collaboration of Caltech, LCOGT, the Weizmann Institute, LBNL, Oxford, Columbia, IPAC, and UC Berkeley. Staff and computational resources were provided by NERSC, supported by the DOE Office of Science. Lick Observatory and the Kast spectrograph are operated by the University of California. HET and its LRS are supported by UT Austin, the Pennsylvania State University, Stanford, Ludwig-Maximilians- Universität München, Georg-August-Universität Göttingen, and the Instituto de Astronomia de la Universidad Nacional Autonoma de Mexico. The EVLA is operated by NRAO for the NSF, under cooperative agreement by Associated Universities, Inc. We thank the staffs of the above observatories for their assistance. A.G. and S.R.K. acknowledge support from the BSF; A.G. further acknowledges support from the ISF, FP7/IRG, Minerva, the Sieff Foundation, and the German–Israeli Fund (GIF). A.V.F. and his group at UC Berkeley acknowledge generous financial assistance from Gary & Cynthia Bengier, the Richard & Rhoda Goldman Fund, the TABASGO Foundation, and NSF grant AST-0908886. A.C. acknowledges support from LIGO, which was constructed by Caltech and MIT with funding from the NSF under cooperative agreementPHY-0757058, and partial support from NASA/Swift grant NNH10ZDA001N.
Group:TAPIR, Palomar Transient Factory, LIGO, Division of Geological and Planetary Sciences
Funders:
Funding AgencyGrant Number
Department of Energy (DOE)UNSPECIFIED
University of TexasUNSPECIFIED
Pennsylvania State UniversityUNSPECIFIED
Stanford UniversityUNSPECIFIED
Ludwig-Maximilians-Universität MünchenUNSPECIFIED
Georg-August-Universität GöttingenUNSPECIFIED
Instituto de Astronomy de la Universidad Nacional Autonoma de MexicoUNSPECIFIED
Binational Science Foundation (USA-Israel)UNSPECIFIED
Israel Science FoundationUNSPECIFIED
European Research Council (ERC)UNSPECIFIED
MinervaUNSPECIFIED
Sieff FoundationUNSPECIFIED
German-Israeli Foundation for Research and DevelopmentUNSPECIFIED
Gary and Cynthia BengierUNSPECIFIED
Richard and Rhoda Goldman FundUNSPECIFIED
TABASGO FoundationUNSPECIFIED
NSFAST-0908886
LIGOUNSPECIFIED
NSFPHY-0757058
NASANNH10ZDA001N
Subject Keywords:supernovae: general; supernovae: individual (PTF 10vgv)
Issue or Number:1
DOI:10.1088/2041-8205/747/1/L5
Record Number:CaltechAUTHORS:20120402-091946766
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20120402-091946766
Official Citation:Evidence for a Compact Wolf-Rayet Progenitor for the Type Ic Supernova PTF 10vgv A. Corsi et al. 2012 ApJ 747 L5
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:29930
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:02 Apr 2012 17:13
Last Modified:09 Nov 2021 19:32

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