Table 4
ALMA continuum models.
| Object | Obs freq.a | Rest freq.a | Total fluxb | Deltac | Gaussianc | FWHMd | Non-thermal | |
|---|---|---|---|---|---|---|---|---|
| (GHz) | (GHz) | (mJy) | (mJy) | (mJy) | (arcsec) | (pc) | fractione | |
| I12112 SW | 231.12 | 247.99 | 0.69 ± 0.05 | ⋯ | 0.69 ± 0.05 | 0.19 ± 0.02 | 260 | 0.43 |
| I12112 NE | 6.81 ± 0.14 | 4.60 ± 0.10 | 2.21 ± 0.10 | 0.35 ± 0.02 | 480 | 0.20 | ||
| I14348 SW | 229.08 | 247.98 | 2.42 ± 0.05 | ⋯ | 2.42 ± 0.05 | 0.17 ± 0.01 | 260 | 0.21 |
| I14348 NE | 1.63 ± 0.05 | ⋯ | 1.63 ± 0.05 | 0.17 ± 0.01 | 270 | 0.21 | ||
| I22491 E | 229.64 | 247.50 | 5.16 ± 0.11 | 4.09 ± 0.06 | 1.07 ± 0.10 | 0.68 ± 0.08 | 1000 | 0.14 |
| I22491 W | <0.14f | ⋯ | ⋯ | ⋯ | ⋯ | ⋯ | ||
Notes. The flux uncertainties are statistical uncertainties from the fit. The absolute flux calibration uncertainty is about 10%. (a) Observed and rest frame continuum frequencies. (b)Total flux of the continuum model. (c)Flux of the delta (unresolved) and Gaussian components of the models. (d) Deconvolved FWHM of the Gaussian component. (e)Non-thermal emission fraction at 248 GHz estimated from the radio 1.49 and 8.44 GHz fluxes (Condon et al. 1990, 1991; see Sect. 3.1.2). (f) 3σ flux upper limit for an unresolved source.
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