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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 7.

Summary of the best-fitting disk densities. Contours corresponding to the 1σ confidence level were determined by interpolation of the ﹩{\chi }_{\nu }^{2}﹩ values over the model grid. The black contours shows the SED fitting and the gray contour shows the Hα fitting, with corresponding colored dots indicating the best-fit model.

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