Table 1 Best-fit parameters for the centroids in the PV diagram using a Gaussian Profile with \(A \exp [-(4\ln 2)(x-x_0)^2/\text {FWHM}^2]\).
From: A magnetized protostellar jet launched from the innermost disk at the truncation radius
Velocity | Amplitude (A) | Peak Position (\(x_0\)) | FWHM |
|---|---|---|---|
(km/s) | (K) | (au) | (au) |
21.01 | 66.93 ± 4.04 | − 1.07 ± 0.84 | 28.35 ± 1.98 |
21.43 | 70.86 ± 4.22 | − 2.07 ± 0.80 | 27.25 ± 1.87 |
21.86 | 75.32 ± 3.25 | − 1.42 ± 0.59 | 27.68 ± 1.38 |
22.28 | 77.74 ± 2.75 | − 0.48 ± 0.47 | 26.95 ± 1.10 |
22.70 | 75.48 ± 2.85 | 0.63 ± 0.49 | 26.41 ± 1.15 |
23.13 | 73.69 ± 2.76 | 0.59 ± 0.46 | 25.09 ± 1.08 |
23.55 | 72.20 ± 1.98 | 0.62 ± 0.33 | 24.50 ± 0.77 |
23.97 | 71.13 ± 1.89 | 1.01 ± 0.33 | 25.58 ± 0.78 |
24.40 | 69.96 ± 2.17 | 1.02 ± 0.37 | 24.07 ± 0.86 |
24.82 | 63.24 ± 2.75 | 1.61 ± 0.43 | 20.37 ± 1.02 |
25.24 | 51.09 ± 3.71 | 1.82 ± 0.70 | 19.71 ± 1.65 |
