Table 1
Parameters of our model with inner disk between Rin and Rsub, where silicates sublimate.
Wavelength | Rsub | Rin | Tin | F∗/Ftot | Fsub/Ftot | F/Ftot | ||
[AU] | [AU] | [K] | [%] | [%] | [%] | |||
|
||||||||
K band | 0.65 | 0.10 | 2400 | 22 | 40 | 38 | ||
H band | ” | ” | ” | 40 | 26 | 34 |
Notes. For both bands, the ratio of the flux contributions from the star (F∗), the ring at dust sublimation (Fsub), and the inner disk (F) to the total flux in the model (Ftot) are reported. The inner disk has a vertical optical depth τ ~ 0.4, and the exponent of the radial temperature profile is α = 0.4.
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