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  5. SN 2011A: A Low-luminosity Interacting Transient with a Double Plateau and Strong Sodium Absorption
 

SN 2011A: A Low-luminosity Interacting Transient with a Double Plateau and Strong Sodium Absorption

Journal
THE ASTROPHYSICAL JOURNAL  
Date Issued
2015
Author(s)
de Jaeger, T.
•
Anderson, J. P.
•
Pignata, G.
•
Hamuy, M.
•
Kankare, E.
•
Stritzinger, M. D.
•
BENETTI, Stefano  
•
BUFANO, FILOMENA  
•
ELIAS DE LA ROSA, NANCY DEL CARMEN  
•
Folatelli, G.
•
Förster, F.
•
González-Gaitán, S.
•
Gutiérrez, C. P.
•
Inserra, C.
•
Kotak, R.
•
Lira, P.
•
Morrell, N.
•
Taddia, F.
•
TOMASELLA, Lina  
DOI
10.1088/0004-637X/807/1/63
Description
The referee is thanked for a through reading of the manuscript, which helped clarify and improve the paper. Support for T.d.J., G.P., M.H., F.F., C.G., F.B., and S.G. is provided by the Ministry of Economy, Development, and Tourism’s Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS. S.G. and F.B. acknowledge support by CONICYT through FONDECYT grants 3130680 and 3120227. S.B. and L.T. are partially supported by the PRIN-INAF 2011 with the project “Transient Universe: from ESO Large to PESSTO.” N.E.R. acknowledges financial support by the MICINN grant AYA2011-24704/ESP, and by the ESF EUROCORES Program EuroGENESIS (MINECO grants EUI2009-04170). M.S. gratefully acknowledges generous support provided by the Danish Agency for Science and Technology and Innovation realized through a Sapere Aude Level 2 grant. E.K. acknowledges financial support from the Jenny and Wihuri Foundation. M.D.S. gratefully acknowledges generous support provided by the Danish Agency for Science and Technology and Innovation realized through a Sapere Aude Level 2 grant. The authors thank J. Mauerhan for providing us with the SN 1994W spectrum (taken from A. Filippenko’s database in Berkeley) and also S.D. Van Dyk for the SN 1997bs spectrum. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration and of data provided by the Central Bureau for Astronomical Telegrams.
Abstract
We present optical photometry and spectroscopy of the optical transient SN 2011A. Our data span 140 days after discovery including {BVRI} u\prime g\prime r\prime i\prime z\prime photometry and 11 epochs of optical spectroscopy. Originally classified as a type IIn supernova (SN IIn) due to the presence of narrow Hα emission, this object shows exceptional characteristics. First, the light curve shows a double plateau, a property only observed before in the impostor SN 1997bs. Second, SN 2011A has a very low luminosity ({M}V=-15.72), placing it between normal luminous SNe IIn and SN impostors. Third, SN 2011A shows low velocity and high equivalent width absorption close to the sodium doublet, which increases with time and is most likely of circumstellar origin. This evolution is also accompanied by a change in line profile; when the absorption becomes stronger, a P Cygni profile appears. We discuss SN 2011A in the context of interacting SNe IIn and SN impostors, which appears to confirm the uniqueness of this transient. While we favor an impostor origin for SN 2011A, we highlight the difficulty in differentiating between terminal and non-terminal interacting transients.

This paper includes data obtained with the 6.5 m Magellan Telescopes and du Pont telescope; the Gemini-North Telescope, Mauna Kea, USA (Gemini Program GN-2010B-Q67, PI: Stritzinger); the PROMPT telescopes at Cerro Tololo Inter-American Observatory in Chile; with the Liverpool Telescope operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council; based on observations made with the Nordic Optical Telescope, operated by the Nordic Optical Telescope Scientific Association at the Observatorio del Roque de los Muchachos, La Palma, Spain, of the Instituto de Astrofisica de Canarias; the NTT from ESO Science Archive Facility under allocations 184.D-1151 and 184.D-1140 (PI: S. Benetti), at the Centro Astronmico Hispano Alemn (CAHA) at Calar Alto, operated jointly by the Max-Planck Institut für Astronomie and the Instituto de Astrofsica de Andaluca (CSIC), on observations collected at Asiago Observatory and the Southern Astrophysical Research (SOAR) telescope, which is a joint project of the Ministério da Ciência, Tecnologia, e Inovação (MCTI) da República Federativa do Brasil, the U.S. National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU).

Volume
807
Issue
1
Start page
63
Uri
http://hdl.handle.net/20.500.12386/24120
Url
https://iopscience.iop.org/article/10.1088/0004-637X/807/1/63
Issn Identifier
0004-637X
Ads BibCode
2015ApJ...807...63D
Rights
open.access
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