Table 2
Parameters for SED modeling.
| T e | EM | Ωff | T thicker | Ωthicker | κ230 GHzΣthicker | T thinner | Ωthinner | κ230 GHzΣthinner | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | |
| (102 K) | (cm-6 pc) | (sr) | (102 K) | (sr) | (102 K) | (sr) | |||
|
|
|||||||||
| FU Ori | 160 | 6.98 × 109 | 1.41 × 10-16 | 3.0 | 1.38 × 10-14 | 103 | 0.6 | 3.88 × 10-12 | 2.06 × 10-2 |
| FU Ori S | 160 | 4.85 × 109 | 1.94 × 10-16 | 3.6 | 5.19 × 10-15 | 32 | 0.6 | 1.04 × 10-12 | 3.87 × 10-2 |
Notes. We use dust opacity index β = 1.75 for the optically thicker and the optically thinner dust components. (1) Electron temperature. (2) Emission measure of the ionized gas component. (3) Solid angle of the ionized gas component. (4) Temperature of the optically thicker dust thermal emission component. (5) Solid angle of the optically thicker dust thermal emission component. 1 sr ~4.25 × 1010 square arcsecond. (6) Dust mass surface density multiplied by the dust opacity at 230 GHz for the optically thicker dust thermal emission component, which is dimensionless. (7) Temperature of the optically thinner dust thermal emission component. (8) Solid angle of the optically thinner dust thermal emission component. (9) Dust mass surface density multiplied by the dust opacity at 230 GHz for the optically thinner dust thermal emission component, which is dimensionless.
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