ALMA, ATCA, and Spitzer observations of the luminous extragalactic supernova SN 1978K

I. A. Smith, S. D. Ryder, R. Kotak, E. C. Kool, S. K. Randall

Research output: Contribution to journalArticlepeer-review

2 Citations (Scopus)
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Abstract

Only three extragalactic supernovae have been detected at late times at millimeter wavelengths: SN 1987A, SN 1978K, and SN 1996cr. SN 1978K is a remarkably luminous Type IIn supernova that remains bright at all wavelengths 40 years after its explosion. Here, we present Atacama Large Millimeter/submillimeter Array (ALMA) observations taken in 2016 using Bands 3, 4, 6, and 7 that show a steepening in the spectrum. An absorbed single power-law model broadly fits all of the radio and millimeter observations, but would require significant chromatic variability. Alternatively, a broken power law fits the radio-millimeter spectrum; this can be explained using an ultra-relativistic spherical blast wave in a wind scaling with a cooling break, as in a gamma-ray burst afterglow. Using updated Australia Telescope Compact Array light curves, we show that the non-thermal radio continuum continues to decay as t -1.53; in the fireball model, this independently defines the power-law indices found in the radio-millimeter spectrum. Supernovae such as SN 1978K might be important contributors to the universal dust budget: only SN 1978K was detected in a search for warm dust in supernovae in the transitional phase (age 10-100 yr). Using Spitzer Space Telescope observations, we show that at least some of this dust emission has been decaying rapidly as t -2.45 over the past decade, suggesting it is being destroyed. Depending on the modeling of the synchrotron emission, the ALMA observations suggest there may be emission from a cold dust component.

Original languageEnglish
Article number59
Pages (from-to)1-10
Number of pages10
JournalAstrophysical Journal
Volume870
Issue number2
DOIs
Publication statusPublished - 10 Jan 2019

Bibliographical note

Copyright 2019 The American Astronomical Society. First published in the Astrophysical journal, 870(2), 59, 2019, published by IOP Publishing. The original publication is available at http://www.doi.org/10.3847/1538-4357/aaf1a3. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.

Keywords

  • galaxies: individual (NGC 1313)
  • gamma-ray burst: general
  • supernovae: general
  • supernovae: individual (SN 1978K)

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