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Probing the 3D Structures of Supernovae through IR Signatures of CO and SiO

  • Authors: T. Mera, P. Hoeflich, C. R. Burns, C. Ashall, K. Medler, E. Fereidouni, W. B. Hoogendam, M. Shahbandeh, S. Shiber, C. M. Pfeffer, E. Baron, J. Lu, N. Morrell, E. Y. Hsiao, M. M. Phillips

T. Mera et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 5.

Same as Figure 4 but with the CO overtone band. Total mass (B) and temperature (C) influence the shape of the overtone more than the other parameters. In panel (A), we show our continuum and have identified a low-bandwidth Mg line profile at 2.475 μm. Changes in the flux level of the continuum will only affect the total mass and temperature profile because they determine the absolute flux levels.

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