Type II-Plateau supernovae as metallicity probes of the Universe

Abstract

We explore a method for metallicity determinations based on quantitative spectroscopy of type II-Plateau (II-P) supernovae (SNe). For consistency, we first evolve a set of 15Msun main sequence stars at 0.1, 0.4, 1, and 2 x the solar metallicity. At the onset of core collapse, we trigger a piston-driven explosion and model the resulting ejecta and radiation. Our theoretical models of such red-supergiant-star explosions at different metallicity show that synthetic spectra of SNe II-P possess optical signatures during the recombination phase that are sensitive to metallicity variations. This sensitivity can be quantified and the metallicity inferred from the strength of metal-line absorptions. Furthermore, these signatures are not limited to O, but also include Na, Ca, Sc, Ti, or Fe. When compared to a sample of SNe II-P from the Carnegie SN Project and previous SN followup programs, we find that most events lie at a metallicity between 0.4 and 2 x solar, with a marked scarcity of SN II-P events at SMC metallicity. This most likely reflects the paucity of low metallicity star forming regions in the local Universe. SNe II-P have high plateau luminosities that make them observable spectroscopically at large distances. Because they exhibit signatures of diverse metal species, in the future they may offer a means to constrain the evolution of the composition (e.g., the O/Fe ratio) in the Universe out to a redshift of one and beyond.

arXiv commentaccepted to MNRAS

References in corpus (36)

• Modules for Experiments in Stellar Astrophysics (MESA)
• The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
• Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars
• [O III]/[N II] as an Abundance Indicator at High Redshift
• Metallicity Calibrations and the Mass-Metallicity Relation for Star-Forming Galaxies
• Using Strong Lines to Estimate Abundances in Extragalactic HII Regions and Starburst Galaxies
• Rotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones
• Long gamma-ray bursts and core-collapse supernovae have different environments
• Determining the Type, Redshift, and Age of a Supernova Spectrum
• Chemo-spectrophotometric evolution of spiral galaxies: I. The model and the Milky Way
• Measured Metallicities at the Sites of Nearby Broad-Lined Type Ic Supernovae and Implications for the SN-GRB Connection
• Type II Supernovae: Model Light Curves and Standard Candle Relationships
• The Carnegie Supernova Project: The Low-Redshift Survey
• Pair Instability Supernovae: Light Curves, Spectra, and Shock Breakout
• Three-Dimensional Simulations of Mixing Instabilities in Supernova Explosions
• Evidence of Environmental Dependencies of Type Ia Supernovae from the Nearby Supernova Factory indicated by Local Hα
• Type II-Plateau supernova radiation: dependencies on progenitor and explosion properties
• Detection of a red supergiant progenitor star of a type II-plateau supernova
• Optical and Infrared Spectroscopy of SN 1999ee and SN 1999ex
• Time Dependent Radiative Transfer Calculations for Supernovae
• Quantitative Spectroscopy of Photospheric-Phase Type II Supernovae
• Progenitor Diagnostics for Stripped Core-Collapse Supernovae: Measured Metallicities at Explosion Sites
• On The Progenitor of the Type II-Plateau Supernova 2003gd in Messier 74
• Radiative Properties of Pair-instability Supernova Explosions
• A Spectroscopic Study of Type Ibc Supernova Host Galaxies from Untargeted Surveys
• Quantitative Spectroscopy of Blue Supergiant Stars in the Disk of M81: Metallicity, Metallicity Gradient and Distance
• Determining the main-sequence mass of Type II supernova progenitors
• Quantitative spectroscopic analysis of and distance to SN1999em
• Observational constraints on the progenitor metallicities of core-collapse supernovae
• Time-dependent Effects in Photospheric-Phase Type II Supernova Spectra
• Strong effects of time-dependent ionization in early SN 1987A
• SN 2003bg: The First Type IIb Hypernova
• The Host Galaxies of Fast-Ejecta Core-Collapse Supernovae
• Reddening, Abundances, and Line Formation in SNe II
• Probing the low-redshift star formation rate as a function of metallicity through the local environments of type II supernovae
• Determination of Primordial Metallicity and Mixing in the Type IIP Supernova 1993W

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