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Panchromatic JWST Observations and Models of the Dim Type Iax Supernova SN 2024vjm at 200 days

  • Authors: E. Baron, J. M. DerKacy, C. Ashall, M. Shahbandeh, Peter H. Hauschildt, T. Barman, J. P. Aufdenberg, C. R. Burns, N. Morrell, M. D. Stritzinger, P. Hoeflich, K. Medler, E. Fereidouni, C. M. Pfeffer, T. Mera, W. B. Hoogendam, S. Shiber, P. J. Brown, Divya Mishra, Inma Dominguez, L. Galbany, Paolo Mazzali, E. Y. Hsiao, Huangfei Xiao, T. de Jaeger, S. Kumar

E. Baron et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 8.

(a) The W7-Iax model shown in Figure 7(a) is compared to the same model but where the molecule opacity has been ignored. Most of the energy comes out in lines due to iron and cobalt near 2 μm. (b) The N1def model shown in Figure 7(b) is compared to the same model but where the molecule opacity has been ignored. Most of the energy comes out in lines due to iron and cobalt near 2 μm.

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