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Table 6
Predicted continuum fluxes for Model 5 at R< 30 AU for diverse values of the astronomical silicates dust mass at 0.2 <R< 30 AU for different grain sizes.
| 0.2 <R< 30 AU | 0.1 <a< 1000 | 0.1 <a< 100 | 0.1 <a< 10 | ||||
| Silicate dust mass | gas/dustinner | 430 μm | 870 μm | 430 μm | 870 μm | 430 μm | 870 μm |
| M ⊙ | mJy | mJy | mJy | mJy | mJy | mJy | |
|
|
|||||||
| 1.0 × 10-7 | 150 | 13.4 | 1.6 | 17.1 | 0.4 | 3.5 | 0.2 |
| 5.0 × 10-8 | 300 | 8.2 | 0.9 | 10.3 | 0.3 | 3.0 | 0.3 |
| 2.5 × 10-8 | 600 | 5.5 | 0.6 | 6.7 | 0.2 | 2.8 | 0.2 |
| 1.0 × 10-8 | 1500 | 3.8 | 0.3 | 4.3 | 0.2 | 2.7 | 0.2 |
| 3.0 × 10-9 | 5000 | 3.0 | 0.2 | 3.2 | 0.2 | 2.7 | 0.2 |
| 1.5 × 10-9 | 10 000 | 2.8 | 0.2 | 3.0 | 0.2 | 2.7 | 0.2 |
| 1.0 × 10-9 | 15 000 | 2.8 | 0.2 | 2.8 | 0.2 | 2.6 | 0.2 |
Notes. The gas mass at R< 30 AU is kept constant and equal to 1.5 × 10-5 M⊙.
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