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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 12.

The same as Figure 10 for the Hα EW. The solid vertical gray line indicates the onset of dissipation, and the dashed gray line indicates when the Hα line was observed to transition to absorption. While the model parameters differ, the constant αT, n = 2.6 scenario with α = 0.4 and Rout = 115 Req is shown for comparison. The colors for each model are consistent with those in Figure 8.

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