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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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
2018 May 16
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 479, Heft: 3, Pages: 3106-3114 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty983 |
| Online-Zugang: | 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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| Verfasserangaben: | Alexandra Kozyreva, Markus Kromer, Ulrich M. Noebauer and Raphael Hirschi |
| Zusammenfassung: | 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 this event. |
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| Beschreibung: | Gesehen am 27.01.2020 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty983 |