Table 2
Best-fit models of the spectral energy distribution using the Robitaille (2017) classification.
| Model set | # of sources | Components | Group |
|---|---|---|---|
| sp––s–i | 12 | star + passive disk; Rinner = Rsub | d |
| sp––h–i | 4 | star + passive disk; variable Rinner | d |
| sp––smi | 5 | star + passive disk + medium; Rinner = Rsub | d |
| sp––hmi | 2 | star + passive disk + medium; variable Rinner | d |
| s–ubsmi | 1 | star + Ulrich envelope + cavity + medium; Rinner =Rsub | e |
| spu–hmi | 1 | star + passive disk + Ulrich envelope + medium; variable Rinner | d+e |
| spubsmi | 1 | star + passive disk + Ulrich envelope + cavity + medium; Rinner = Rsub | d+e |
Notes. The model set names are from Robitaille (2017). Seven characters in the model set names indicate which component is present; they are (in order): s: star; p: passive disk, p or u: power-law or Ulrich envelope; b: bipolar cavities; h: inner hole; m: ambient medium; and i: interstellar dust. A dash (-) is used when a component is absent. Rinner is the inner radius for the disk, envelope, and the ambient medium – when one or more of these components are present. Rsub is the dust sublimation radius.
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