The Astrophysical Journal Letters (Jan 2023)

A JWST Near- and Mid-infrared Nebular Spectrum of the Type Ia Supernova 2021aefx

  • Lindsey A. Kwok,
  • Saurabh W. Jha,
  • Tea Temim,
  • Ori D. Fox,
  • Conor Larison,
  • Yssavo Camacho-Neves,
  • Max J. Brenner Newman,
  • Justin D. R. Pierel,
  • Ryan J. Foley,
  • Jennifer E. Andrews,
  • Carles Badenes,
  • Barnabas Barna,
  • K. Azalee Bostroem,
  • Maxime Deckers,
  • Andreas Flörs,
  • Peter Garnavich,
  • Melissa L. Graham,
  • Or Graur,
  • Griffin Hosseinzadeh,
  • D. Andrew Howell,
  • John P. Hughes,
  • Joel Johansson,
  • Sarah Kendrew,
  • Wolfgang E. Kerzendorf,
  • Keiichi Maeda,
  • Kate Maguire,
  • Curtis McCully,
  • John T. O’Brien,
  • Armin Rest,
  • David J. Sand,
  • Melissa Shahbandeh,
  • Louis-Gregory Strolger,
  • Tamás Szalai,
  • Chris Ashall,
  • E. Baron,
  • Chris R. Burns,
  • James M. DerKacy,
  • Tyco Mera Evans,
  • Alec Fisher,
  • Lluís Galbany,
  • Peter Hoeflich,
  • Eric Hsiao,
  • Thomas de Jaeger,
  • Emir Karamehmetoglu,
  • Kevin Krisciunas,
  • Sahana Kumar,
  • Jing Lu,
  • Justyn Maund,
  • Paolo A. Mazzali,
  • Kyle Medler,
  • Nidia Morrell,
  • Mark. M. Phillips,
  • Benjamin J. Shappee,
  • Maximilian Stritzinger,
  • Nicholas Suntzeff,
  • Charles Telesco,
  • Michael Tucker,
  • Lifan Wang

DOI
https://doi.org/10.3847/2041-8213/acb4ec
Journal volume & issue
Vol. 944, no. 1
p. L3

Abstract

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We present JWST near-infrared (NIR) and mid-infrared (MIR) spectroscopic observations of the nearby normal Type Ia supernova (SN) SN 2021aefx in the nebular phase at +255 days past maximum light. Our Near Infrared Spectrograph (NIRSpec) and Mid Infrared Instrument observations, combined with ground-based optical data from the South African Large Telescope, constitute the first complete optical+NIR+MIR nebular SN Ia spectrum covering 0.3–14 μ m. This spectrum unveils the previously unobserved 2.5−5 μ m region, revealing strong nebular iron and stable nickel emission, indicative of high-density burning that can constrain the progenitor mass. The data show a significant improvement in sensitivity and resolution compared to previous Spitzer MIR data. We identify numerous NIR and MIR nebular emission lines from iron-group elements as well as lines from the intermediate-mass element argon. The argon lines extend to higher velocities than the iron-group elements, suggesting stratified ejecta that are a hallmark of delayed-detonation or double-detonation SN Ia models. We present fits to simple geometric line profiles to features beyond 1.2 μ m and find that most lines are consistent with Gaussian or spherical emission distributions, while the [Ar iii ] 8.99 μ m line has a distinctively flat-topped profile indicating a thick spherical shell of emission. Using our line profile fits, we investigate the emissivity structure of SN 2021aefx and measure kinematic properties. Continued observations of SN 2021aefx and other SNe Ia with JWST will be transformative to the study of SN Ia composition, ionization structure, density, and temperature, and will provide important constraints on SN Ia progenitor and explosion models.

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