The Type IIn Supernova SN 2010bt: The Explosion of a Star in Outburst

Nancy Elias-Rosa, Schuyler D. Van Dyk, Stefano Benetti, Enrico Cappellaro, Nathan Smith, Rubina Kotak, Massimo Turatto, Alexei V. Filippenko, Giuliano Pignata, Ori D. Fox, Lluis Galbany, Santiago González-Gaitán, Matteo Miluzio, L. A.G. Monard, Mattias Ergon

Research output: Contribution to journalArticle

2 Citations (Scopus)

Abstract

It is well known that massive stars (M > 8 M ) evolve up to the collapse of the stellar core, resulting in most cases in a supernova (SN) explosion. Their heterogeneity is related mainly to different configurations of the progenitor star at the moment of the explosion and to their immediate environments. We present photometry and spectroscopy of SN 2010bt, which was classified as a Type IIn SN from a spectrum obtained soon after discovery and was observed extensively for about 2 months. After the seasonal interruption owing to its proximity to the Sun, the SN was below the detection threshold, indicative of a rapid luminosity decline. We can identify the likely progenitor with a very luminous star (log L/L ≈ 7) through comparison of Hubble Space Telescope images of the host galaxy prior to explosion with those of the SN obtained after maximum light. Such a luminosity is not expected for a quiescent star, but rather for a massive star in an active phase. This progenitor candidate was later confirmed via images taken in 2015 (∼5 yr post-discovery), in which no bright point source was detected at the SN position. Given these results and the SN behavior, we conclude that SN 2010bt was likely a Type IIn SN and that its progenitor was a massive star that experienced an outburst shortly before the final explosion, leading to a dense H-rich circumstellar environment around the SN progenitor.

Original languageEnglish (US)
Article number68
JournalAstrophysical Journal
Volume860
Issue number1
DOIs
StatePublished - Jun 10 2018

Fingerprint

outburst
supernovae
explosions
explosion
stars
massive stars
point source
spectroscopy
luminosity
stellar cores
interruption
Hubble Space Telescope
point sources
photometry
proximity
sun
galaxies
moments
thresholds
configurations

Keywords

  • galaxies: individual (NGC 7130)
  • stars: evolution
  • supernovae: general
  • supernovae: individual (SN 2010bt)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Elias-Rosa, N., Van Dyk, S. D., Benetti, S., Cappellaro, E., Smith, N., Kotak, R., ... Ergon, M. (2018). The Type IIn Supernova SN 2010bt: The Explosion of a Star in Outburst. Astrophysical Journal, 860(1), [68]. https://doi.org/10.3847/1538-4357/aac510

The Type IIn Supernova SN 2010bt : The Explosion of a Star in Outburst. / Elias-Rosa, Nancy; Van Dyk, Schuyler D.; Benetti, Stefano; Cappellaro, Enrico; Smith, Nathan; Kotak, Rubina; Turatto, Massimo; Filippenko, Alexei V.; Pignata, Giuliano; Fox, Ori D.; Galbany, Lluis; González-Gaitán, Santiago; Miluzio, Matteo; Monard, L. A.G.; Ergon, Mattias.

In: Astrophysical Journal, Vol. 860, No. 1, 68, 10.06.2018.

Research output: Contribution to journalArticle

Elias-Rosa, N, Van Dyk, SD, Benetti, S, Cappellaro, E, Smith, N, Kotak, R, Turatto, M, Filippenko, AV, Pignata, G, Fox, OD, Galbany, L, González-Gaitán, S, Miluzio, M, Monard, LAG & Ergon, M 2018, 'The Type IIn Supernova SN 2010bt: The Explosion of a Star in Outburst', Astrophysical Journal, vol. 860, no. 1, 68. https://doi.org/10.3847/1538-4357/aac510
Elias-Rosa N, Van Dyk SD, Benetti S, Cappellaro E, Smith N, Kotak R et al. The Type IIn Supernova SN 2010bt: The Explosion of a Star in Outburst. Astrophysical Journal. 2018 Jun 10;860(1). 68. https://doi.org/10.3847/1538-4357/aac510
Elias-Rosa, Nancy ; Van Dyk, Schuyler D. ; Benetti, Stefano ; Cappellaro, Enrico ; Smith, Nathan ; Kotak, Rubina ; Turatto, Massimo ; Filippenko, Alexei V. ; Pignata, Giuliano ; Fox, Ori D. ; Galbany, Lluis ; González-Gaitán, Santiago ; Miluzio, Matteo ; Monard, L. A.G. ; Ergon, Mattias. / The Type IIn Supernova SN 2010bt : The Explosion of a Star in Outburst. In: Astrophysical Journal. 2018 ; Vol. 860, No. 1.
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