Table 4
Results from SED fitting.
| Parameter | Best fit valuesa | |
| Source #1 | Source #8 | |
|
|
||
| Stellar mass (M⊙) | 10.7 (+0, –0.2) | 6.7 |
| Stellar age (yr) | 3.0 (+0, –0.2) × 104 | 6.0 × 105 |
| Stellar radius (R⊙) | 33.6 (+4.5, –0) | 3.1 |
| Stellar temperature (K) | 7840 (+0, –625) | 19950 |
| Disk mass (M⊙) | 1.3 (+0, –0.3) × 10-2 | 3.6 × 10-3 |
| Disk accretion rate (M⊙ yr-1) | 2.9 (+0, –2.42) × 10-6 | 7.6 × 10-7 |
| Disk/envelope inner radius (AU) | 8.4 (+2.2, –0) | 12.7 |
| Disk outer radius (AU) | 16.1 (+1.2, –0) | 134 |
| Envelope mass (M⊙) | 6.1 (+0.5, –0) × 102 | 2.3 |
| Envelope accretion rate (M⊙ yr-1) | 9.3 (+1.1, –0) × 10-4 | 7.5 × 10-7 |
| Envelope outer radius (AU) | 1.0 × 105 | 4.3 × 104 |
| Total Luminosity (L⊙) | 3.9 (+0.3, –0) × 103 | 1.4 × 103 |
| Angle of inclination of the disk axisb (°) | 31.8 ( ± 18.5) | 49.5 (+14.6, –8.1) |
| AV (Foreground) | 16.1 (+4.7, –0.8) | 17.1 (+0, –0.5) |
| AV (Circumstellar) | 25.4 (+0, –8.7) | 0.6 (+0, –0.1) |
Notes.
The values given in parenthesis are the differences in the parameters of the additional models with (
) per data point <3, from those of the best fit model. No errors are given when the parameters of these models do not differ; nevertheless, the uncertainties could be higher as described in Sect. 3.2. A distance of 4.01 kpc is used.
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