Measured metallicities at the sites of nearby broad-lined type Ic supernovae and implications for the supernovae gamma-ray burst connection

M. Modjaz, L. Kewley, R. P. Kirshner, K. Z. Stanek, P. Challis, P. M. Garnavich, J. E. Greene, P. L. Kelly, J. L. Prieto

    Research output: Contribution to journalArticle

    Abstract

    We compare the chemical abundances at the sites of 12 nearby (z < 0.14) Type Ic supernovae (SN Ic) that showed broad lines, but had no observed gamma-ray burst (GRB), with the chemical abundances in five nearby (z < 0.25) galaxies at the sites of GRBs where broad-lined SN Ic were seen after the fireball had faded. It has previously been noted that GRB hosts are low in luminosity and low in their metal abundances. If low metallicity is sufficient to force the evolution of massive stars to end their lives as GRBs with an accompanying broad-lined SN Ic, then we would expect higher metal abundances for the broad-lined SN Ic that have no detected GRBs. This is what we observe, and this trend is independent of the choice of metallicity calibration we adopt and the mode of SN survey that found the broad-lined SN Ic. A unique feature of this analysis is that we present new spectra of the host galaxies and analyze all measurements of both samples in the same set of methods, using the galaxy emission-line measurements corrected for extinction and stellar absorption, via independent metallicity diagnostics of Kewley & Dopita, McGaugh, and Pettini & Pagel. In our small sample, the boundary between galaxies that have GRBs accompanying their broad-lined SN Ic and those that have broad-lined SN Ic without GRBs lies at an oxygen abundance of 12 + log(O/H)KD02 8.5, which corresponds to 0.2-0.6 Z depending on the adopted metallicity scale and solar abundance value. Even when we limit the comparison to SN Ic that were found in untargeted supernova surveys, the environment of every broad-lined SN Ic that had no GRB is more metal rich than the site of any broad-lined SN Ic where a GRB was detected.

    Original languageEnglish (US)
    Pages (from-to)1136-1150
    Number of pages15
    JournalAstronomical Journal
    Volume135
    Issue number4
    DOIs
    StatePublished - Apr 1 2008

    Fingerprint

    gamma ray bursts
    metallicity
    supernovae
    galaxies
    metal
    metals
    fireballs
    massive stars
    extinction
    luminosity
    calibration
    trends
    oxygen

    Keywords

    • Galaxies: abundances
    • Galaxies: distances and redshifts
    • Gamma rays: bursts
    • Supernovae: general

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

    Cite this

    Modjaz, M., Kewley, L., Kirshner, R. P., Stanek, K. Z., Challis, P., Garnavich, P. M., ... Prieto, J. L. (2008). Measured metallicities at the sites of nearby broad-lined type Ic supernovae and implications for the supernovae gamma-ray burst connection. Astronomical Journal, 135(4), 1136-1150. https://doi.org/10.1088/0004-6256/135/4/1136

    Measured metallicities at the sites of nearby broad-lined type Ic supernovae and implications for the supernovae gamma-ray burst connection. / Modjaz, M.; Kewley, L.; Kirshner, R. P.; Stanek, K. Z.; Challis, P.; Garnavich, P. M.; Greene, J. E.; Kelly, P. L.; Prieto, J. L.

    In: Astronomical Journal, Vol. 135, No. 4, 01.04.2008, p. 1136-1150.

    Research output: Contribution to journalArticle

    Modjaz, M, Kewley, L, Kirshner, RP, Stanek, KZ, Challis, P, Garnavich, PM, Greene, JE, Kelly, PL & Prieto, JL 2008, 'Measured metallicities at the sites of nearby broad-lined type Ic supernovae and implications for the supernovae gamma-ray burst connection', Astronomical Journal, vol. 135, no. 4, pp. 1136-1150. https://doi.org/10.1088/0004-6256/135/4/1136
    Modjaz, M. ; Kewley, L. ; Kirshner, R. P. ; Stanek, K. Z. ; Challis, P. ; Garnavich, P. M. ; Greene, J. E. ; Kelly, P. L. ; Prieto, J. L. / Measured metallicities at the sites of nearby broad-lined type Ic supernovae and implications for the supernovae gamma-ray burst connection. In: Astronomical Journal. 2008 ; Vol. 135, No. 4. pp. 1136-1150.
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    abstract = "We compare the chemical abundances at the sites of 12 nearby (z < 0.14) Type Ic supernovae (SN Ic) that showed broad lines, but had no observed gamma-ray burst (GRB), with the chemical abundances in five nearby (z < 0.25) galaxies at the sites of GRBs where broad-lined SN Ic were seen after the fireball had faded. It has previously been noted that GRB hosts are low in luminosity and low in their metal abundances. If low metallicity is sufficient to force the evolution of massive stars to end their lives as GRBs with an accompanying broad-lined SN Ic, then we would expect higher metal abundances for the broad-lined SN Ic that have no detected GRBs. This is what we observe, and this trend is independent of the choice of metallicity calibration we adopt and the mode of SN survey that found the broad-lined SN Ic. A unique feature of this analysis is that we present new spectra of the host galaxies and analyze all measurements of both samples in the same set of methods, using the galaxy emission-line measurements corrected for extinction and stellar absorption, via independent metallicity diagnostics of Kewley & Dopita, McGaugh, and Pettini & Pagel. In our small sample, the boundary between galaxies that have GRBs accompanying their broad-lined SN Ic and those that have broad-lined SN Ic without GRBs lies at an oxygen abundance of 12 + log(O/H)KD02 8.5, which corresponds to 0.2-0.6 Z⊙ depending on the adopted metallicity scale and solar abundance value. Even when we limit the comparison to SN Ic that were found in untargeted supernova surveys, the environment of every broad-lined SN Ic that had no GRB is more metal rich than the site of any broad-lined SN Ic where a GRB was detected.",
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    AU - Kewley, L.

    AU - Kirshner, R. P.

    AU - Stanek, K. Z.

    AU - Challis, P.

    AU - Garnavich, P. M.

    AU - Greene, J. E.

    AU - Kelly, P. L.

    AU - Prieto, J. L.

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