Figure 14 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 14.

Hα emission line dissipation modeled with the constant αT, n = 2.6 scenario. The thick, dark lines correspond to observations. The thinner, lighter lines are models using constant α and isothermal disks with α = 0.4 and R_out = 115 R_eq. The 0 yr model corresponds to ρ₀ = 2.5 × 10⁻¹¹ g cm⁻³ and n = 2.6.

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