Open Access

Table A.3.

Parameters of all the 22 GHz H2O maser features detected around VLA1 (epoch 2016.45).

(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) (°)
VLA1.2.01 -18.441 1.366 - 57.07 ± 1.42 12.29 0.66 2.2 ± 0.2 −72 ± 10 3.5 −676 ± 102
VLA1.2.02 -11.915 -9.304 - 0.29 ± 0.02 16.40 0.76
VLA1.2.03 -9.052 -3.773 - 659.23 ± 2.17 9.48 0.66 0.7 ± 0.1 −73 ± 4
VLA1.2.04 -4.210 0.237 - 13.25 ± 0.42 7.82 1.99
VLA1.2.05 -3.873 0.980 - 47.27 ± 0.64 8.98 0.75 1.3 ± 0.1 −76 ± 15
VLA1.2.06 -1.810 18.555 - 134.08 ± 1.61 10.14 0.70
VLA1.2.07 0 0 - 1619.87 ± 4.42 10.92 1.19 0.8 ± 0.1 −59 ± 3
VLA1.2.08 11.452 12.955 - 25.57 ± 0.86 9.27 1.14
VLA1.2.09 26.945 32.818 - 330.99 ± 2.28 10.35 0.58
VLA1.2.10 33.892 21.893 - 24.05 ± 0.72 13.43 3.68
VLA1.2.11 35.366 44.006 - 10.46 ± 0.23 9.00 1.21
VLA1.2.12 36.124 22.461 - 35.42 ± 1.19 9.29 0.81
VLA1.2.13 37.723 21.629 - 412.53 ± 1.48 12.69 1.10 1.0 ± 0.1 −65 ± 16
VLA1.2.14 38.144 21.221 - 98.05 ± 4.33 10.82 1.31 1.2 ± 0.4 −11 ± 14
VLA1.2.15 41.765 25.604 - 28.31 ± 0.73 13.40 0.80
VLA1.2.16 42.691 0.790 - 0.24 ± 0.02 2.68 0.49
VLA1.2.17 47.112 24.559 - 150.64 ± 0.68 13.51 1.05 2.1 ± 0.5 −56 ± 3
VLA1.2.18 48.923 25.745 - 35.99 ± 0.84 13.56 0.91
VLA1.2.19 49.301 24.933 - 4.04 ± 0.64 15.72 1.05
VLA1.2.20 155.146 73.784 - 3.72 ± 0.21 13.64 1.09

Notes.

a

The reference position is α2000 = 20h38m36s​.43403 ± 0s​.00011 and δ2000 = +42° 37′34″​​.8667 ± 0″​​.0010.

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 ∼ 3136 K (Γν = 17 s−1) TbΔΩ has to be adjusted by adding +1.3 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.

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