OGLE14-073: a promising pair-instability supernova candidate

The recently discovered bright Type II supernova OGLE14-073 evolved very slowly. The light curve rose to maximum for 90 d from discovery and then declined at a rate compatible with the radioactive decay of 56Co. In this study, we show that a pair-instability supernova is a plausible mechanism for th...

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Main Authors: Kozyreva, Alexandra (Author) , Kromer, Markus (Author)
Format: Article (Journal)
Language:English
Published: 2018 May 16
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 479, Issue: 3, Pages: 3106-3114
ISSN:1365-2966
DOI:10.1093/mnras/sty983
Online Access:Resolving-System, Volltext: https://doi.org/10.1093/mnras/sty983
Verlag: https://academic.oup.com/mnras/article/479/3/3106/4996805
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Author Notes:Alexandra Kozyreva, Markus Kromer, Ulrich M. Noebauer and Raphael Hirschi

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