Fig. 6

Radial profiles of protostellar accretion disk models. Top panel: disk photospheric temperature for non-irradiated disk (lower solid line) and irradiated disk (upper solid line) for m∗ = 10 M⊙ with fiducial accretion rate. The equivalent models for m∗ = 10 M⊙ with accretion rate enhanced by a factor of 10 are shown by the dotted lines. The equivalent models for m∗ = 20 M⊙ with fiducial accretion rate are shown by the dashed lines. The long-dashed horizontal lines show the approximate range of temperatures where we consider there are contributions to the CO bandhead equivalent width. Bottom panel: Keplerian velocities for the m∗ = 10, 20 M⊙ models, shown by the solid and dashed lines, respectively.
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