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Table 3
Best-fit parameters of the temperature-gradient models.
| khalo |
|
|
T1,in (K) | q1 | r1,in (AU) | Δr1 (AU) | T2,in (K) | q2 | r2,in (AU) | Δr2 (AU) |
|
||||
|
|
|||||||||||||||
| one-component | 0.306 | 60 | 33 | 800 | 0.63 | 0.392 | 5.0 | 10.7 | |||||||
|
|
|||||||||||||||
| two-component |
|
 a
|
|
|
0.5b |
|
|
|
|
|
|
1.15 | |||
Notes.
(b)
The power-law index q1 was fixed to 0.5 (corresponding to a flared irradiated disk; Kenyon & Hartmann 1987), since q1 cannot be constrained because of the small radial thickness of the inner disk ring (see Appendix A.3).
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