Table 3
Best-fit models of SED using the Robitaille (2017) classification.
| Model Set | # of sources | Components | Group |
|---|---|---|---|
| s–s-i | 4 | star | − |
| sp–s-i | 2 | star + passive disk; Rinner = Rsub | d |
| sp–h-i | 4 | star + passive disk; variable Rinner | d |
| s-pbhmi | 1 | star + power-law envelope + cavity + medium; variable Rinner | e |
| spubsmi | 1 | star + passive disk + Ulrich envelope + cavity + medium; Rinner = Rsub | d + e |
Notes. 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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