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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 7.

(a) A simple model, W7-Iax, using W7 abundances with an ejecta mass of 0.42 M⊙ and the velocities reduced by a factor of 10 (the W7-Iax model). This model has isothermal ejecta with T = 2000 K, and γ-ray deposition from the (reduced) radioactive nickel is included. (b) The N1def model. This model has isothermal ejecta with T = 2000 K and includes γ-ray deposition.

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