Observed SED of GW Ori. The broad band photometry is shown with the filled circles, and the IRS spectrum of this source is displayed in solid line. The thick gray line shows a best-fit model. The dashed line shows the model SED for a disk with M_disk = 0.14 M_⊙, H_out/R_out = 0.235, and R_in = 2.3 AU, and the dot-dashed line display another model SED for a disk with M_disk = 0.14 M_⊙, H_out/R_out = 0.2, and R_in = 8 AU. The photospheric emission level is indicated with a thin gray curve.