Figure 11 from The Be Star 66 Ophiuchi: 60 Years of Disk Evolution

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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 11.

The same as Figure 10, but for the Hα line profile. The simulated lines were convolved using the Gaussian determined to give the best fit in Figure 4. The models from the constant αT, n = 3.5 and n = 2.6 scenarios lie on top of the NRES/LCOGT 2020 observation and in absorption. The colors for each model are consistent with those in Figure 8.

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