Multi-wavelength observations of the enduring type IIn Supernovae 2005ip and 2006jd

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Multi-wavelength observations of the enduring type IIn Supernovae 2005ip and 2006jd. / Stritzinger, Maximilian; Taddia, Francesco; Fransson, Claes; Fox, Ori D.; Morrell, Nidia; Phillips, M.M.; Sollerman, Jesper; Anderson, J.P.; Boldt, Luis; Brown, Peter J.; Campillay, Abdo; Castellon, Sergio; Contreras, Carlos; Folatelli, Gaston; Habergham, S. M.; Hamuy, Mario; Hjorth, Jens; James, Phil A.; Krzeminski, Wojtek; Mattila, Seppo; Persson, Sven E.; Roth, Miguel.

In: The Astrophysical Journal, Vol. 756, No. 2, 173, 2012.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Stritzinger, M, Taddia, F, Fransson, C, Fox, OD, Morrell, N, Phillips, MM, Sollerman, J, Anderson, JP, Boldt, L, Brown, PJ, Campillay, A, Castellon, S, Contreras, C, Folatelli, G, Habergham, SM, Hamuy, M, Hjorth, J, James, PA, Krzeminski, W, Mattila, S, Persson, SE & Roth, M 2012, 'Multi-wavelength observations of the enduring type IIn Supernovae 2005ip and 2006jd', The Astrophysical Journal, vol. 756, no. 2, 173. https://doi.org/10.1088/0004-637X/756/2/173

APA

Stritzinger, M., Taddia, F., Fransson, C., Fox, O. D., Morrell, N., Phillips, M. M., ... Roth, M. (2012). Multi-wavelength observations of the enduring type IIn Supernovae 2005ip and 2006jd. The Astrophysical Journal, 756(2), [173]. https://doi.org/10.1088/0004-637X/756/2/173

Vancouver

Stritzinger M, Taddia F, Fransson C, Fox OD, Morrell N, Phillips MM et al. Multi-wavelength observations of the enduring type IIn Supernovae 2005ip and 2006jd. The Astrophysical Journal. 2012;756(2). 173. https://doi.org/10.1088/0004-637X/756/2/173

Author

Stritzinger, Maximilian ; Taddia, Francesco ; Fransson, Claes ; Fox, Ori D. ; Morrell, Nidia ; Phillips, M.M. ; Sollerman, Jesper ; Anderson, J.P. ; Boldt, Luis ; Brown, Peter J. ; Campillay, Abdo ; Castellon, Sergio ; Contreras, Carlos ; Folatelli, Gaston ; Habergham, S. M. ; Hamuy, Mario ; Hjorth, Jens ; James, Phil A. ; Krzeminski, Wojtek ; Mattila, Seppo ; Persson, Sven E. ; Roth, Miguel. / Multi-wavelength observations of the enduring type IIn Supernovae 2005ip and 2006jd. In: The Astrophysical Journal. 2012 ; Vol. 756, No. 2.

Bibtex

@article{eb6528eaf9b54d11b1c209a00717c9f7,
title = "Multi-wavelength observations of the enduring type IIn Supernovae 2005ip and 2006jd",
abstract = "We present an observational study of the Type IIn supernovae (SNe IIn) 2005ip and 2006jd. Broadband UV, optical, and near-IR photometry, and visual-wavelength spectroscopy of SN 2005ip complement and extend upon published observations to 6.5 years past discovery. Our observations of SN 2006jd extend from UV to mid-infrared wavelengths, and like SN 2005ip, are compared to reported X-ray measurements to understand the nature of the progenitor. Both objects display a number of similarities with the 1988Z-like subclass of SN IIn including (1) remarkably similar early-and late-phase optical spectra, (2) a variety of high-ionization coronal lines, (3) long-duration optical and near-IR emission, and (4) evidence of cold and warm dust components. However, diversity is apparent, including an unprecedented late-time r-band excess in SN 2006jd. The observed differences are attributed to differences between the mass-loss history of the progenitor stars. We conclude that the progenitor of SN 2006jd likely experienced a significant mass-loss event during its pre-SN evolution akin to the great 19th century eruption of. Carinae. Contrarily, as advocated by Smith et al., the circumstellar environment of SN 2005ip is found to be more consistent with a clumpy wind progenitor.",
author = "Maximilian Stritzinger and Francesco Taddia and Claes Fransson and Fox, {Ori D.} and Nidia Morrell and M.M. Phillips and Jesper Sollerman and J.P. Anderson and Luis Boldt and Brown, {Peter J.} and Abdo Campillay and Sergio Castellon and Carlos Contreras and Gaston Folatelli and Habergham, {S. M.} and Mario Hamuy and Jens Hjorth and James, {Phil A.} and Wojtek Krzeminski and Seppo Mattila and Persson, {Sven E.} and Miguel Roth",
year = "2012",
doi = "10.1088/0004-637X/756/2/173",
language = "English",
volume = "756",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - Multi-wavelength observations of the enduring type IIn Supernovae 2005ip and 2006jd

AU - Stritzinger, Maximilian

AU - Taddia, Francesco

AU - Fransson, Claes

AU - Fox, Ori D.

AU - Morrell, Nidia

AU - Phillips, M.M.

AU - Sollerman, Jesper

AU - Anderson, J.P.

AU - Boldt, Luis

AU - Brown, Peter J.

AU - Campillay, Abdo

AU - Castellon, Sergio

AU - Contreras, Carlos

AU - Folatelli, Gaston

AU - Habergham, S. M.

AU - Hamuy, Mario

AU - Hjorth, Jens

AU - James, Phil A.

AU - Krzeminski, Wojtek

AU - Mattila, Seppo

AU - Persson, Sven E.

AU - Roth, Miguel

PY - 2012

Y1 - 2012

N2 - We present an observational study of the Type IIn supernovae (SNe IIn) 2005ip and 2006jd. Broadband UV, optical, and near-IR photometry, and visual-wavelength spectroscopy of SN 2005ip complement and extend upon published observations to 6.5 years past discovery. Our observations of SN 2006jd extend from UV to mid-infrared wavelengths, and like SN 2005ip, are compared to reported X-ray measurements to understand the nature of the progenitor. Both objects display a number of similarities with the 1988Z-like subclass of SN IIn including (1) remarkably similar early-and late-phase optical spectra, (2) a variety of high-ionization coronal lines, (3) long-duration optical and near-IR emission, and (4) evidence of cold and warm dust components. However, diversity is apparent, including an unprecedented late-time r-band excess in SN 2006jd. The observed differences are attributed to differences between the mass-loss history of the progenitor stars. We conclude that the progenitor of SN 2006jd likely experienced a significant mass-loss event during its pre-SN evolution akin to the great 19th century eruption of. Carinae. Contrarily, as advocated by Smith et al., the circumstellar environment of SN 2005ip is found to be more consistent with a clumpy wind progenitor.

AB - We present an observational study of the Type IIn supernovae (SNe IIn) 2005ip and 2006jd. Broadband UV, optical, and near-IR photometry, and visual-wavelength spectroscopy of SN 2005ip complement and extend upon published observations to 6.5 years past discovery. Our observations of SN 2006jd extend from UV to mid-infrared wavelengths, and like SN 2005ip, are compared to reported X-ray measurements to understand the nature of the progenitor. Both objects display a number of similarities with the 1988Z-like subclass of SN IIn including (1) remarkably similar early-and late-phase optical spectra, (2) a variety of high-ionization coronal lines, (3) long-duration optical and near-IR emission, and (4) evidence of cold and warm dust components. However, diversity is apparent, including an unprecedented late-time r-band excess in SN 2006jd. The observed differences are attributed to differences between the mass-loss history of the progenitor stars. We conclude that the progenitor of SN 2006jd likely experienced a significant mass-loss event during its pre-SN evolution akin to the great 19th century eruption of. Carinae. Contrarily, as advocated by Smith et al., the circumstellar environment of SN 2005ip is found to be more consistent with a clumpy wind progenitor.

U2 - 10.1088/0004-637X/756/2/173

DO - 10.1088/0004-637X/756/2/173

M3 - Journal article

VL - 756

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 173

ER -

ID: 49743436