Image Details
Caption: Fig. 8.
Star+disk models of the 10 stars considered for more sophisticated modeling; see text for discussion as to how they were selected and the details of the modeling. Notation is as in Figs. 1–4: the ﹩x﹩‐axis plots the log of the wavelength in microns, and the ﹩y﹩‐axis plots ﹩\mathrm{log}\,( \lambda F_{\lambda }) ﹩ in cgs units (ergs s−1 cm−2). Points gleaned from the literature are diamonds, boxes are detections or upper limits from IRAS, and circles are new MIPS points. Downward‐pointing arrows indicate upper limits.
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