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The Be Star 66 Ophiuchi: 60 Years of Disk Evolution

  • Authors: K. C. Marr, C. E. Jones, A. C. Carciofi, A. C. Rubio, B. C. Mota, M. R. Ghoreyshi, D. W. Hatfield, and L. R. Rímulo

2021 The Astrophysical Journal 912 76.

  • Provider: AAS Journals

Caption: Figure 10.

SEDs for each of the dynamical scenarios after dissipation. For comparison the best-fitting initial steady state is shown. The observed data are the same as that presented in Figure 6. The two models from the variable αT scenarios lie on top of each other. The colors for each model are consistent with those in Figure 8.

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