A JWST Medium Resolution MIRI Spectrum and Models of the Type Ia supernova 2021aefx at +415 d

Type Ia supernovae High Energy Astrophysical Phenomena (astro-ph.HE) FOS: Physical sciences Astrophysics 01 natural sciences 520 QB460-466 Supernovae Astrophysics - Solar and Stellar Astrophysics http://astrothesaurus.org/uat/1728 0103 physical sciences [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Astrophysics - High Energy Astrophysical Phenomena Solar and Stellar Astrophysics (astro-ph.SR) http://astrothesaurus.org/uat/1668
DOI: 10.48550/arxiv.2404.17043 Publication Date: 2024-04-25
ABSTRACT
We present a JWST MIRI/MRS spectrum (5-27 $\mathrm{\mu}$m) of the Type Ia supernova (SN Ia), SN 2021aefx at $+415$ days past $B$-band maximum. The spectrum, which was obtained during iron-dominated nebular phase, has been analyzed in combination with previous observations 2021aefx, to provide first time series analysis an Ia. find temporal evolution [Co III] 11.888 $\mathrm{\mu}$m feature directly traces decay $^{56}$Co. spectra, line profiles, and their are off-center delayed-detonation models. Best fits were White Dwarf (WD) central densities $\rho_c=0.9-1.1\times 10^9$g cm$^{-3}$, WD mass M$_{\mathrm{WD}}$=1.33-1.35M$_\odot$, magnetic field $\approx10^6$G, deflagration-to-detonation transition $\approx$ 0.5 $M_\odot$ seen opposite sight observer. inner electron capture core is dominated by energy deposition from $\gamma$-rays whereas broader region positron deposition, placing +415 d transitional phase positron-dominated regime. formerly `flat-tilted' profile 9 now significant contribution [Ni IV], [Fe II], less [Ar III], alters shape as positrons excite mostly low-velocity Ar. Overall, strength stable Ni features transport rather than mass. Based on multi-dimensional models, our strongly supports single-spot, close-to-central ignition indication for pre-existing turbulent velocity field, excludes multiple-spot, ignition.
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