Table 4
Parameters of the five best fit models to the IRAS 18264-1152 SED.
| χ2 | Mc | Σ | Rcore | m* | θview | AV | Menv | θw,esc | Ṁdisc | Lbol,iso | Lbol |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (M⊙) | (g cm-2) | (pc) (′′) | (M⊙) | (°) | (mag) | (M⊙) | (°) | (M⊙ yr−1) | (L⊙) | (L⊙) | |
| 1.28 | 120 | 3.160 | 0.05 (3.1) | 4 | 13 | 222.87 | 113.23 | 11 | 5.7 × 10−4 | 4.0 × 104 | 1.1 × 104 |
| 1.51 | 160 | 3.160 | 0.05 (3.1) | 4 | 13 | 220.74 | 153.10 | 9 | 6.1 × 10−4 | 3.2 × 104 | 1.2 × 104 |
| 1.57 | 100 | 3.160 | 0.04 (2.5) | 4 | 13 | 224.33 | 92.43 | 12 | 5.4 × 10−4 | 4.8 × 104 | 1.0 × 104 |
| 1.68 | 200 | 3.160 | 0.06 (3.8) | 4 | 13 | 192.65 | 191.38 | 7 | 6.5 × 10−4 | 2.5 × 104 | 1.2 × 104 |
| 1.98 | 480 | 0.316 | 0.29 (18.8) | 8 | 13 | 172.32 | 461.98 | 8 | 2.0 × 10−4 | 1.9 × 104 | 9.4 × 103 |
Notes. From left to right, the parameters are: χ2, initial core mass, mean mass surface density of the clump, initial core radius, current protostellar mass, viewing angle, foreground extinction, current envelope mass, half opening angle of outflow cavity, accretion rate from disc to protostar, isotropic bolometric luminosity, intrinsic bolometric luminosity.
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