Table 2
Overview of the best RADMC-3D model parameters.
| Parameter | Inner disk | Outer disk |
|
|
||
| rin [au]∗ | 0.07a | 30 |
| rout [au]∗ | 0.11a | 60 |
| rc [au] | – | 50b |
| Mdust [M⊙] | 2 × 10-11 a | 9 × 10-5 b |
| δ | 1 | 1 |
| H0/r0 | 0.02/0.1a | 4/50b |
| β | 1 | 1 |
|
|
||
| {amin, amax} [μm]∗ | {0.01, 1000} | {0.01, 1000} |
| ~10 | ~10 | |
| p | –3.5 | –3.5 |
|
|
||
| incl [deg]∗ | 69 | 69 |
| PA [deg]∗ | 114 | 114 |
Notes. δ denotes the exponent of the surface density power-law and β corresponds to the disk flaring index. For the radiation source we take the following star parameters: Teff = 5400 K, M = 1.5 M⊙, R = 1.3 R⊙, where the star is assumed to be spherical. All parameters marked with an asterisk symbol (∗) were varied during the radiative transfer modeling. The grain size distributions as well as inclination and PA were taken to be the same for the inner and outer disk.
Reference.
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