An extremely energetic supernova from a very massive star in a dense medium

Matt Nicholl*, Peter K. Blanchard, Edo Berger, Ryan Chornock, Raffaella Margutti, Sebastian Gomez, Ragnhild Lunnan, Adam A. Miller, Wen fai Fong, Giacomo Terreran, Alejandro Vigna-Gómez, Kornpob Bhirombhakdi, Allyson Bieryla, Pete Challis, Russ R. Laher, Frank J. Masci, Kerry Paterson

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

11 Scopus citations

Abstract

The interaction of a supernova with a circumstellar medium (CSM) can dramatically increase the emitted luminosity by converting kinetic energy to thermal energy. In ‘superluminous’ supernovae of type IIn—named for narrow hydrogen lines1 in their spectra—the integrated emission can reach2–6 ~1051 erg, attainable by thermalizing most of the kinetic energy of a conventional supernova. A few transients in the centres of active galaxies have shown similar spectra and even larger energies7,8, but are difficult to distinguish from accretion onto the supermassive black hole. Here we present a new event, SN2016aps, offset from the centre of a low-mass galaxy, that radiated ≳5 × 1051 erg, necessitating a hyper-energetic supernova explosion. We find a total (supernova ejecta + CSM) mass likely exceeding 50−100 M, with energy ≳1052 erg, consistent with some models of pair-instability supernovae or pulsational pair-instability supernovae—theoretically predicted thermonuclear explosions from helium cores >50 M. Independent of the explosion mechanism, this event demonstrates the existence of extremely energetic stellar explosions, detectable at very high redshifts, and provides insight into dense CSM formation in the most massive stars.

Original languageEnglish (US)
Pages (from-to)893-899
Number of pages7
JournalNature Astronomy
Volume4
Issue number9
DOIs
StatePublished - Sep 1 2020

ASJC Scopus subject areas

  • Astronomy and Astrophysics

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