What powers the 3000-day light curve of SN 2006gy?

Ori D. Fox, Nathan Smith, S. Mark Ammons, Jennifer Andrews, K. Azalee Bostroem, S. Bradley Cenko, Geoffrey C. Clayton, Eli Dwek, Alexei V. Filippenko, Joseph S. Gallagher, Patrick L. Kelly, Jon C. Mauerhan, Adam A. Miller, Schuyler D. Van Dyk

Research output: Contribution to journalArticle

8 Citations (Scopus)

Abstract

SN 2006gy was the most luminous supernova (SN) ever observed at the time of its discovery and the first of the newly defined class of superluminous supernovae (SLSNe). The extraordinary energetics of SN 2006gy and all SLSNe (>1051 erg) require either atypically large explosion energies (e.g. pair-instability explosion) or the efficient conversion of kinetic into radiative energy (e.g. shock interaction). The mass-loss characteristics can therefore offer important clues regarding the progenitor system. For the case of SN 2006gy, both a scattered and thermal light echo from circumstellar material (CSM) have been reported at later epochs (day ~800), ruling out the likelihood of a pair-instability event and leading to constraints on the characteristics of the CSM. Owing to the proximity of the SN to the bright host-galaxy nucleus, continued monitoring of the light echo has not been trivial, requiring the high resolution offered by the Hubble Space Telescope (HST) or ground-based adaptive optics (AO). Here, we report detections of SN 2006gy using HST and Keck AO at ~3000 d post-explosion and consider the emission mechanism for the very late-time light curve.While the optical light curve and optical spectral energy distribution are consistent with a continued scattered-light echo, a thermal echo is insufficient to power the K'-band emission by day 3000. Instead, we present evidence for late-time infrared emission from dust that is radiatively heated by CSM interaction within an extremely dense dust shell, and we consider the implications on the CSM characteristics and progenitor system.

Original languageEnglish (US)
Pages (from-to)4366-4378
Number of pages13
JournalMonthly Notices of the Royal Astronomical Society
Volume454
Issue number4
DOIs
StatePublished - 2015

Fingerprint

light curve
supernovae
explosion
echoes
explosions
dust
energy
adaptive optics
Hubble Space Telescope
erg
energetics
shell
spectral energy distribution
extremely high frequencies
kinetics
material
proximity
monitoring
shock
time measurement

Keywords

  • Circumstellar matter
  • Dust
  • Extinction
  • Infrared: stars
  • Supernovae: general
  • Supernovae: individual: SN 2006gy

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Fox, O. D., Smith, N., Mark Ammons, S., Andrews, J., Azalee Bostroem, K., Bradley Cenko, S., ... Van Dyk, S. D. (2015). What powers the 3000-day light curve of SN 2006gy? Monthly Notices of the Royal Astronomical Society, 454(4), 4366-4378. https://doi.org/10.1093/mnras/stv2270

What powers the 3000-day light curve of SN 2006gy? / Fox, Ori D.; Smith, Nathan; Mark Ammons, S.; Andrews, Jennifer; Azalee Bostroem, K.; Bradley Cenko, S.; Clayton, Geoffrey C.; Dwek, Eli; Filippenko, Alexei V.; Gallagher, Joseph S.; Kelly, Patrick L.; Mauerhan, Jon C.; Miller, Adam A.; Van Dyk, Schuyler D.

In: Monthly Notices of the Royal Astronomical Society, Vol. 454, No. 4, 2015, p. 4366-4378.

Research output: Contribution to journalArticle

Fox, OD, Smith, N, Mark Ammons, S, Andrews, J, Azalee Bostroem, K, Bradley Cenko, S, Clayton, GC, Dwek, E, Filippenko, AV, Gallagher, JS, Kelly, PL, Mauerhan, JC, Miller, AA & Van Dyk, SD 2015, 'What powers the 3000-day light curve of SN 2006gy?', Monthly Notices of the Royal Astronomical Society, vol. 454, no. 4, pp. 4366-4378. https://doi.org/10.1093/mnras/stv2270
Fox OD, Smith N, Mark Ammons S, Andrews J, Azalee Bostroem K, Bradley Cenko S et al. What powers the 3000-day light curve of SN 2006gy? Monthly Notices of the Royal Astronomical Society. 2015;454(4):4366-4378. https://doi.org/10.1093/mnras/stv2270
Fox, Ori D. ; Smith, Nathan ; Mark Ammons, S. ; Andrews, Jennifer ; Azalee Bostroem, K. ; Bradley Cenko, S. ; Clayton, Geoffrey C. ; Dwek, Eli ; Filippenko, Alexei V. ; Gallagher, Joseph S. ; Kelly, Patrick L. ; Mauerhan, Jon C. ; Miller, Adam A. ; Van Dyk, Schuyler D. / What powers the 3000-day light curve of SN 2006gy?. In: Monthly Notices of the Royal Astronomical Society. 2015 ; Vol. 454, No. 4. pp. 4366-4378.
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AU - Bradley Cenko, S.

AU - Clayton, Geoffrey C.

AU - Dwek, Eli

AU - Filippenko, Alexei V.

AU - Gallagher, Joseph S.

AU - Kelly, Patrick L.

AU - Mauerhan, Jon C.

AU - Miller, Adam A.

AU - Van Dyk, Schuyler D.

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KW - Extinction

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KW - Supernovae: general

KW - Supernovae: individual: SN 2006gy

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