SN 2008iy

An unusual Type IIn Supernova with an enduring 400-d rise time

A. A. Miller, J. M. Silverman, Nathaniel Butler, J. S. Bloom, R. Chornock, A. V. Filippenko, M. Ganeshalingam, C. R. Klein, W. Li, P. E. Nugent, N. Smith, T. N. Steele

Research output: Contribution to journalArticle

38 Citations (Scopus)

Abstract

We present spectroscopic and photometric observations of the Type IIn supernova (SN) 2008iy. SN 2008iy showed an unprecedentedly long rise time of ~400 d, making it the first known SN to take significantly longer than 100 d to reach peak optical luminosity. The peak absolute magnitude of SN 2008iy was Mr ≈ -19.1 mag, and the total radiated energy over the first ~700 d was ~2 × 1050 erg. Spectroscopically, SN 2008iy is very similar to the Type IIn SN 1988Z at late times and, like SN 1988Z, it is a luminous X-ray source (both SNe had an X-ray luminosity LX > 1041 erg s-1). SN 2008iy has a growing near-infrared excess at late times similar to several other SNe IIn. The Hα emission-line profile of SN 2008iy shows a narrow P Cygni absorption component, implying a pre-SN wind speed of ~100 km s-1. We argue that the luminosity of SN 2008iy is powered via the interaction of the SN ejecta with a dense, clumpy circumstellar medium. The ~400-d rise time can be understood if the number density of clumps increases with distance over a radius ~1.7 × 1016 cm from the progenitor. This scenario is possible if the progenitor experienced an episodic phase of enhanced mass loss <1 century prior to explosion or if the progenitor wind speed increased during the decades before core collapse. We favour the former scenario, which is reminiscent of the eruptive mass-loss episodes observed for luminous blue variable (LBV) stars. The progenitor wind speed and increased mass-loss rates serve as further evidence that at least some, and perhaps all, Type IIn SNe experience LBV-like eruptions shortly before core collapse.We also discuss the host galaxy of SN 2008iy, a subluminous dwarf galaxy, and offer a few reasons why the recent suggestion that unusual, luminous SNe preferentially occur in dwarf galaxies may be the result of observational biases.

Original languageEnglish (US)
Pages (from-to)305-317
Number of pages13
JournalMonthly Notices of the Royal Astronomical Society
Volume404
Issue number1
DOIs
StatePublished - May 2010
Externally publishedYes

Fingerprint

supernovae
wind velocity
erg
ejecta
explosion
near infrared
volcanic eruption
luminosity
dwarf galaxies
energy
loss
blue stars
variable stars
clumps
volcanic eruptions
suggestion
explosions
x rays
galaxies
radii

Keywords

  • Circumstellar matter
  • General
  • Individual
  • Mass-loss
  • SN 1988Z
  • SN 2008iy
  • Stars
  • Supernovae

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Miller, A. A., Silverman, J. M., Butler, N., Bloom, J. S., Chornock, R., Filippenko, A. V., ... Steele, T. N. (2010). SN 2008iy: An unusual Type IIn Supernova with an enduring 400-d rise time. Monthly Notices of the Royal Astronomical Society, 404(1), 305-317. https://doi.org/10.1111/j.1365-2966.2010.16280.x

SN 2008iy : An unusual Type IIn Supernova with an enduring 400-d rise time. / Miller, A. A.; Silverman, J. M.; Butler, Nathaniel; Bloom, J. S.; Chornock, R.; Filippenko, A. V.; Ganeshalingam, M.; Klein, C. R.; Li, W.; Nugent, P. E.; Smith, N.; Steele, T. N.

In: Monthly Notices of the Royal Astronomical Society, Vol. 404, No. 1, 05.2010, p. 305-317.

Research output: Contribution to journalArticle

Miller, AA, Silverman, JM, Butler, N, Bloom, JS, Chornock, R, Filippenko, AV, Ganeshalingam, M, Klein, CR, Li, W, Nugent, PE, Smith, N & Steele, TN 2010, 'SN 2008iy: An unusual Type IIn Supernova with an enduring 400-d rise time', Monthly Notices of the Royal Astronomical Society, vol. 404, no. 1, pp. 305-317. https://doi.org/10.1111/j.1365-2966.2010.16280.x
Miller, A. A. ; Silverman, J. M. ; Butler, Nathaniel ; Bloom, J. S. ; Chornock, R. ; Filippenko, A. V. ; Ganeshalingam, M. ; Klein, C. R. ; Li, W. ; Nugent, P. E. ; Smith, N. ; Steele, T. N. / SN 2008iy : An unusual Type IIn Supernova with an enduring 400-d rise time. In: Monthly Notices of the Royal Astronomical Society. 2010 ; Vol. 404, No. 1. pp. 305-317.
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abstract = "We present spectroscopic and photometric observations of the Type IIn supernova (SN) 2008iy. SN 2008iy showed an unprecedentedly long rise time of ~400 d, making it the first known SN to take significantly longer than 100 d to reach peak optical luminosity. The peak absolute magnitude of SN 2008iy was Mr ≈ -19.1 mag, and the total radiated energy over the first ~700 d was ~2 × 1050 erg. Spectroscopically, SN 2008iy is very similar to the Type IIn SN 1988Z at late times and, like SN 1988Z, it is a luminous X-ray source (both SNe had an X-ray luminosity LX > 1041 erg s-1). SN 2008iy has a growing near-infrared excess at late times similar to several other SNe IIn. The Hα emission-line profile of SN 2008iy shows a narrow P Cygni absorption component, implying a pre-SN wind speed of ~100 km s-1. We argue that the luminosity of SN 2008iy is powered via the interaction of the SN ejecta with a dense, clumpy circumstellar medium. The ~400-d rise time can be understood if the number density of clumps increases with distance over a radius ~1.7 × 1016 cm from the progenitor. This scenario is possible if the progenitor experienced an episodic phase of enhanced mass loss <1 century prior to explosion or if the progenitor wind speed increased during the decades before core collapse. We favour the former scenario, which is reminiscent of the eruptive mass-loss episodes observed for luminous blue variable (LBV) stars. The progenitor wind speed and increased mass-loss rates serve as further evidence that at least some, and perhaps all, Type IIn SNe experience LBV-like eruptions shortly before core collapse.We also discuss the host galaxy of SN 2008iy, a subluminous dwarf galaxy, and offer a few reasons why the recent suggestion that unusual, luminous SNe preferentially occur in dwarf galaxies may be the result of observational biases.",
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AU - Bloom, J. S.

AU - Chornock, R.

AU - Filippenko, A. V.

AU - Ganeshalingam, M.

AU - Klein, C. R.

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N2 - We present spectroscopic and photometric observations of the Type IIn supernova (SN) 2008iy. SN 2008iy showed an unprecedentedly long rise time of ~400 d, making it the first known SN to take significantly longer than 100 d to reach peak optical luminosity. The peak absolute magnitude of SN 2008iy was Mr ≈ -19.1 mag, and the total radiated energy over the first ~700 d was ~2 × 1050 erg. Spectroscopically, SN 2008iy is very similar to the Type IIn SN 1988Z at late times and, like SN 1988Z, it is a luminous X-ray source (both SNe had an X-ray luminosity LX > 1041 erg s-1). SN 2008iy has a growing near-infrared excess at late times similar to several other SNe IIn. The Hα emission-line profile of SN 2008iy shows a narrow P Cygni absorption component, implying a pre-SN wind speed of ~100 km s-1. We argue that the luminosity of SN 2008iy is powered via the interaction of the SN ejecta with a dense, clumpy circumstellar medium. The ~400-d rise time can be understood if the number density of clumps increases with distance over a radius ~1.7 × 1016 cm from the progenitor. This scenario is possible if the progenitor experienced an episodic phase of enhanced mass loss <1 century prior to explosion or if the progenitor wind speed increased during the decades before core collapse. We favour the former scenario, which is reminiscent of the eruptive mass-loss episodes observed for luminous blue variable (LBV) stars. The progenitor wind speed and increased mass-loss rates serve as further evidence that at least some, and perhaps all, Type IIn SNe experience LBV-like eruptions shortly before core collapse.We also discuss the host galaxy of SN 2008iy, a subluminous dwarf galaxy, and offer a few reasons why the recent suggestion that unusual, luminous SNe preferentially occur in dwarf galaxies may be the result of observational biases.

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