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  1. OA@INAF
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12386/29467
Title: Observations of Type Ia Supernova 2014J for Nearly 900 Days and Constraints on Its Progenitor System
Authors: Li, Wenxiong
Wang, Xiaofeng
Hu, Maokai
Yang, Yi
Zhang, Jujia
Mo, Jun
Chen, Zhihao
Zhang, Tianmeng
BENETTI, Stefano 
CAPPELLARO, Enrico 
ELIAS DE LA ROSA, NANCY DEL CARMEN 
Isern, Jordi
Morales-Garoffolo, Antonia
Huang, Fang
OCHNER, PAOLO
PASTORELLO, Andrea
REGUITTI, ANDREA
TARTAGLIA, LEONARDO 
Terreran, Giacomo
TOMASELLA, Lina 
Wang, Lifan
Issue Date: 2019
Journal: THE ASTROPHYSICAL JOURNAL 
Number: 882
Issue: 1
First Page: 30
Abstract: We present extensive ground-based and Hubble Space Telescope (HST) photometry of the highly reddened, very nearby SN Ia 2014J in M82, covering the phases from 9 days before to about 900 days after the B-band maximum. SN 2014J is similar to other normal SNe Ia near the maximum light, but it shows flux excess in the B band in the early nebular phase. This excess flux emission can be due to light scattering by some structures of circumstellar materials located at a few 10<SUP>17</SUP> cm, consistent with a single-degenerate progenitor system or a double-degenerate progenitor system with mass outflows in the final evolution or magnetically driven winds around the binary system. At t ∼ +300 to ∼+500 days past the B-band maximum, the light curve of SN 2014J shows a faster decline relative to the <SUP>56</SUP>Ni decay. That feature can be attributed to the significant weakening of the emission features around [Fe III] λ4700 and [Fe II] λ5200 rather than the positron escape, as previously suggested. Analysis of the HST images taken at t > 600 days confirms that the luminosity of SN 2014J maintains a flat evolution at the very late phase. Fitting the late-time pseudobolometric light curve with radioactive decay of <SUP>56</SUP>Ni, <SUP>57</SUP>Ni, and <SUP>55</SUP>Fe isotopes, we obtain the mass ratio <SUP>57</SUP>Ni/<SUP>56</SUP>Ni as 0.035 ± 0.011, which is consistent with the corresponding value predicted from the 2D and 3D delayed-detonation models. Combined with early-time analysis, we propose that delayed-detonation through the single-degenerate scenario is most likely favored for SN 2014J.
URI: http://hdl.handle.net/20.500.12386/29467
URL: https://iopscience.iop.org/article/10.3847/1538-4357/ab2b49
ISSN: 0004-637X
DOI: 10.3847/1538-4357/ab2b49
Bibcode ADS: 2019ApJ...882...30L
Fulltext: open
Appears in Collections:1.01 Articoli in rivista

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