Table 2
Parameters in the models.
| Object | Ṁ (M⊙ yr −1) | Rsub,min (R⋆) | Rk (R⋆) | ⟨Fobs⟩(erg cm−2 s−1) | i(deg) | δ |
|---|---|---|---|---|---|---|
| Mon-660 | 3 × 10−9 | 7.7 | 7.64 | 9.51 × 10−12 | 71 | 0.15 |
| Mon-660 | 3 × 10−9 | 7.7 | 7.64 | 9.51 × 10−12 | 72 | 0.15 |
| Mon-660 | 3 × 10−9 | 7.7 | 7.64 | 9.51 × 10−12 | 73 | 0.17 |
| Mon-660 | 3 × 10−9 | 7.7 | 7.64 | 9.51 × 10−12 | 74 | 0.15 |
| Mon-660 | 3 × 10−9 | 7.7 | 7.64 | 9.51 × 10−12 | 75 | 0.14 |
| Mon-660 | 3 × 10−9 | 7.7 | 7.64 | 9.51 × 10−12 | 76 | 0.15 |
| Mon-660 | 3 × 10−9 | 7.7 | 7.64 | 9.51 × 10−12 | 77 | 0.16 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 67 | 0.03 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 68 | 0.02 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 69 | 0.0 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 70 | 0.0 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 71 | 0.02 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 72 | 0.03 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 73 | 0.03 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 74 | 0.03 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 75 | 0.01 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 76 | 0.02 |
| Mon-811 | 3 × 10−9 | 6.19 | 8.19 | 8.65 × 10−12 | 77 | 0.05 |
| Mon-1140 | 7.76 × 10−9 | 7.93 | 6.75 | 3.76 × 10−12 | 73-77 | 0.01 |
| Mon-1308 | 8.51 × 10−9 | 5.45 | 7.81 | 2.77 × 10−12 | 69 | 0.2 |
| Mon-1308 | 8.51 × 10−9 | 5.45 | 7.81 | 2.77 × 10−12 | 70 | 0.25 |
| Mon-1308 | 8.51 × 10−9 | 5.45 | 7.81 | 2.77 × 10−12 | 71 | 0.4 |
| Mon-1308 | 8.51 × 10−9 | 5.45 | 7.81 | 2.77 × 10−12 | 72 | 0.45 |
| Mon-1308 | 8.51 × 10−9 | 5.45 | 7.81 | 2.77 × 10−12 | 73 | 0.35 |
| Mon-1308 | 8.51 × 10−9 | 5.45 | 7.81 | 2.77 × 10−12 | 74 | 0.38 |
| Mon-1308 | 8.51 × 10−9 | 5.45 | 7.81 | 2.77 × 10−12 | 75 | 0.4 |
| Mon-1308 | 8.51 × 10−9 | 5.45 | 7.81 | 2.77 × 10−12 | 76 | 0.4 |
| Mon-1308 | 8.51 × 10−9 | 5.45 | 7.81 | 2.77 × 10−12 | 77 | 0.56 |
Notes. The first column shows the object name. The second column corresponds to the mass accretion rate. The third column is the minimum sublimation radius. The forth column is the keplerian radius. The fifth column is the observed flux at 4.5 μm. The sixth column corresponds to the inclination. The seventh column is the δ parameter (see text for details).
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