Table 4.
ℐBG, 𝒱BG values for all models obtained in the second fitting step (three parameters) directly compared to the ℐsha, 𝒱sha used for visual aid in Fig. 7, and to the average values of ℐ and 𝒱 from the ALMA data.
| Model ID | IBG (Jy) | VBG (Jy) | Isha (Jy) | Vsha (Jy) |
|---|---|---|---|---|
| nc_db_k | 2.01 | −0.036 | 1.75 | −0.025 |
| nc_fb_k | 4.27 | +0.34 | 1.75 | −0.025 |
| c_db_k | 1.73 | −0.028 | 1.75 | −0.025 |
| c_fb_k | 3.63 | +0.025 | 1.75 | −0.025 |
| nc_db_nk | 1.24 | −0.022 | 1.75 | −0.028 |
| nc_fb_nk | 2.86 | +0.24 | 1.75 | −0.028 |
| c_db_nk | 1.4 | −0.021 | 1.75 | −0.025 |
| c_fb_nk | 3.4 | +0.20 | 1.75 | −0.025 |
| ALMA average | 1.90 | −0.027 | 1.90 | −0.027 |
Notes. The average of ℐ is from the first 10 points since the later increase in Stokes Isha is argued to occur due to the time evolution of the background or the spot-background interactions.
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