Figure 5 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 5.

Change in the Hα EW and corresponding ﹩{\chi }_{\nu }^{2}﹩ values for the best-fit model with increases in outer disk radius. The parameter ﹩{\chi }_{\nu }^{2}﹩ was computed as the fit of the convolved profile to the HPOL 1989 line profile.

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