Table 3.
Model fitting results from the RadioAstron image.
| Component | S | FWHM | r | PA | Tb, obs |
|---|---|---|---|---|---|
| ID | (Jy) | (mas) | (mas) | (°) | (K) |
| Core | 6.40 ± 0.64 | 0.10 ± 0.01 | 0 | 0 | (1.6 ± 0.2) × 1012 |
| C1 | 1.04 ± 0.10 | 0.13 ± 0.01 | 0.13 ± 0.01 | 11.3 ± 1.2 | (1.5 ± 0.2) × 1011 |
| C2 | 0.29 ± 0.02 | 0.09 ± 0.01 | 0.57 ± 0.03 | 36.9 ± 3.3 | (8.8 ± 0.9) × 1010 |
| C3 | 1.58 ± 0.15 | 0.30 ± 0.01 | 0.86 ± 0.02 | 32.3 ± 3.3 | (4.3 ± 0.4) × 1010 |
| E | 0.68 ± 0.07 | 1.64 ± 0.02 | 2.26 ± 0.01 | 36.6 ± 3.4 | (6.2 ± 0.6) × 108 |
Notes. From left to right, the columns show the component ID, flux density in Jy, size of the component in mas, radial distance from the core in mas, position angle of the component position with respect to the core in degrees (origin in north and positive counterclockwise direction), and the observed brightness temperature without Doppler and redshift correction in Kelvin (K).
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