Supernova 2020wnt: An Atypical Superluminous Supernova with a Hidden Central Engine
We present observations of a peculiar hydrogen- and helium-poor stripped-envelope (SE) supernova (SN) 2020wnt, primarily in the optical and near-infrared (near-IR). Its peak absolute bolometric magnitude of −20.9 mag ( L bol, peak = (6.8 ± 0.3) × 10 43 erg s −1 ) and a rise time of 69 days are remin...
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Veröffentlicht in: | The Astrophysical journal 2023-07, Vol.951 (1), p.34 |
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Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
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Zusammenfassung: | We present observations of a peculiar hydrogen- and helium-poor stripped-envelope (SE) supernova (SN) 2020wnt, primarily in the optical and near-infrared (near-IR). Its peak absolute bolometric magnitude of −20.9 mag (
L
bol, peak
= (6.8 ± 0.3) × 10
43
erg s
−1
) and a rise time of 69 days are reminiscent of hydrogen-poor superluminous SNe (SLSNe I), luminous transients potentially powered by spinning-down magnetars. Before the main peak, there is a brief peak lasting |
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ISSN: | 0004-637X 1538-4357 1538-4357 |
DOI: | 10.3847/1538-4357/acc6c3 |