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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 8.

Optical depth of Model P at day 385 for the local peaks of the vibrational modes of the CO overtone (scaled) and fundamental bands if clumps are not included. If clumps are included, then the optical depth is ray-dependent.

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