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

Kwok, LA, Jha, SW, Temim, T, Fox, OD, Larison, C, Camacho-Neves, Y, Brenner Newman, MJ, Pierel, JDR, Foley, RJ, Andrews, JE, Badenes, C, Barna, B, Bostroem, KA, Deckers, M, Flörs, A, Garnavich, P, Graham, ML, Graur, O, Hosseinzadeh, G, Howell, DA , Hughes, JP, Johansson, J, Kendrew, S, Kerzendorf, WE, Maeda, K, Maguire, K, McCully, C, O’Brien, JT, Rest, A, Sand, DJ, Shahbandeh, M, Strolger, LG, Szalai, T, Ashall, C, Baron, E, Burns, CR, DerKacy, JM, Evans, TM, Fisher, A, Galbany, L, Hoeflich, P, Hsiao, E, de Jaeger, T, Karamehmetoglu, E, Krisciunas, K, Kumar, S, Lu, J, Maund, J, Mazzali, PA, Medler, K, Morrell, N, Phillips, MM, Shappee, BJ, Stritzinger, M, Suntzeff, N, Telesco, C, Tucker, M and Wang, L (2023) A JWST Near- and Mid-infrared Nebular Spectrum of the Type Ia Supernova 2021aefx. Astrophysical Journal Letters, 944 (1). ISSN 2041-8205

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Open Access URL: https://doi.org/10.3847/2041-8213/acb4ec (Published version)


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 μm. This spectrum unveils the previously unobserved 2.5−5 μm 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 μm and find that most lines are consistent with Gaussian or spherical emission distributions, while the [Ar iii] 8.99 μm 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.

Item Type: Article
Uncontrolled Keywords: 0201 Astronomical and Space Sciences; Astronomy & Astrophysics
Subjects: Q Science > QB Astronomy
Q Science > QC Physics
Divisions: Astrophysics Research Institute
Publisher: American Astronomical Society
SWORD Depositor: A Symplectic
Date Deposited: 16 Mar 2023 12:10
Last Modified: 16 Mar 2023 12:15
DOI or ID number: 10.3847/2041-8213/acb4ec
URI: https://researchonline.ljmu.ac.uk/id/eprint/19119
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