Open Access

Table A.5.

Parameters of all the 22 GHz H2O maser features detected around VLA1 (epoch 2018.44).

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
Maser RAa Deca Zone Peak Vlsr ΔvL Pl χ ΔVib TbΔΩb PV B|| θc
feature offset offset Intensity (I)
(mas) (mas) (Jy/beam) (km/s) (km/s) (%) (°) (km/s) (log K sr) (%) (mG) (°)
VLA1.3.01 -68.500 -88.299 - 2.13 ± 0.14 12.90 0.82
VLA1.3.02 -27.156 -18.986 - 36.76 ± 0.53 10.74 0.92
VLA1.3.03 -0.463 -1.347 - 17.56 ± 0.12 11.82 1.29 1.1 ± 0.1 −83 ± 2 < 0.4
VLA1.3.04 0 0 - 446.25 ± 4.18 8.63 1.10 0.7 ± 0.1 −88 ± 6 1.6 −764 ± 115
VLA1.3.05 2.147 -2.552 - 2.08 ± 0.10 11.98 1.45
VLA1.3.06 3.705 5.379 - 283.86 ± 1.56 9.58 1.14 0.8 ± 0.1 +88 ± 5
VLA1.3.07 3.705 5.184 - 265.98 ± 1.73 9.56 1.15 0.9 ± 0.1 +81 ± 6
VLA1.3.08 10.526 12.749 - 21.66 ± 0.18 7.77 1.16
VLA1.3.09 12.673 14.587 - 11.87 ± 0.31 11.45 0.80 1.0 ± 0.1 −82 ± 3
VLA1.3.10 19.872 18.551 - 8.22 ± 0.14 10.77 1.60
VLA1.3.11 21.514 45.429 - 21.83 ± 0.16 14.96 0.92 10.6 ± 0.2 +86 ± 6
VLA1.3.12 23.703 22.160 - 67.31 ± 1.06 9.98 1.01 0.8 ± 0.3 +88 ± 7
VLA1.3.13 62.479 31.822 - 7.38 ± 0.18 13.59 1.88
VLA1.3.14 63.532 63.618 - 4.04 ± 0.31 11.32 0.93
VLA1.3.15 63.827 65.319 - 48.05 ± 0.57 10.66 0.94 1.1 ± 0.1 −86 ± 7
VLA1.3.16 65.721 32.665 - 29.64 ± 0.23 13.30 1.10 0.9 ± 0.1 −88 ± 4 1.6 −733 ± 113
VLA1.3.17 81.467 32.475 - 4.71 ± 0.39 11.09 0.82
VLA1.3.18 84.120 31.231 - 33.10 ± 0.42 11.11 0.80 1.1 ± 0.1 −85 ± 4
VLA1.3.19 86.856 31.273 - 11.23 ± 0.55 10.80 0.87 1.7 ± 0.1 −88 ± 7
VLA1.3.20 94.814 42.259 - 18.33 ± 0.22 13.38 0.99 1.0 ± 0.1 −88 ± 6

Notes.

a

The reference position is α2000 = 20h38m36s​.43201 ± 0s​.00008 and δ2000 = 42° 37′34″​​.34.8588 ± 0″​​.0009.

b

The best-fitting results obtained by using a model based on the radiative transfer theory of H2O masers for Γ + Γν = 1 s−1 S11a. The errors were determined by analyzing the full probability distribution function. For T ∼ 2916 K (Γν = 15 s−1) TbΔΩ has to be adjusted by adding +1.2 log K sr (Anderson & Watson 1993).

c

The angle between the magnetic field and the maser propagation direction is determined by using the observed Pl and the fitted emerging brightness temperature. The errors were determined by analyzing the full probability distribution function. The boldface indicates that |θ+ − 55°| < |θ − 55°|, i.e., the magnetic field is parallel to the linear polarization vector (see Sect. 2).

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