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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 10.

For given initial temperature structures of Models P (left) and O (right, Figure 3) we show our best-fit SiO fundamental bands for prolate (P), oblate (O), and nonclumping (S) models. The continuum used for day 285 shows the identification of a low-bandwidth H line profile at 8.75 μm that overlaps our high-bandwidth molecular feature. Also included in the continuum but not plotted is the edge of the [Ni I] line at 7.5 μm. For parameter values, see Table 2.

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