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Table A.1.

Parameters of all the 22 GHz H2O maser features detected around VLA1 (epoch 2014.46).

(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) (°)
VLA1.1.01 -101.803 -153.618 - 0.43 ± 0.03 8.37 0.38
VLA1.1.02 -101.761 -156.307 - 0.57 ± 0.04 8.48 0.44
VLA1.1.03 -64.879 -93.826 - 2.59 ± 0.17 12.77 0.52 15.6 ± 2.0 +48 ± 3 < 0.4
VLA1.1.04 -31.619 -19.016 - 15.85 ± 0.15 12.61 2.88 10.1 ± 2.5 −62 ± 1
VLA1.1.05 -28.672 -99.377 - 86.37 ± 1.06 10.61 2.31 2.3 ± 0.6 −25 ± 4 0.5
VLA1.1.06 -24.588 -99.083 - 8.37 ± 0.34 11.35 1.45
VLA1.1.07 -23.703 -12.516 - 74.21 ± 0.79 10.98 0.58
VLA1.1.08 -14.778 -1.484 - 23.15 ± 0.04 8.63 0.57 1.3 ± 0.1 −39 ± 3
VLA1.1.09 -10.610 -10.700 - 1.71 ± 0.02 7.90 2.81
VLA1.1.10 -7.621 -6.420 - 61.34 ± 0.35 9.77 2.10
VLA1.1.11 -6.821 -9.647 - 44.38 ± 0.13 12.48 1.22 0.7 ± 0.1 −45 ± 5
VLA1.1.12 -5.810 -6.111 - 34.60 ± 0.21 9.56 0.58
VLA1.1.13 -4.084 -9.914 - 0.54 ± 0.01 16.77 3.61
VLA1.1.14 1.684 1.221 - 9.01 ± 0.20 9.53 0.87
VLA1.1.15 0 0 - 1205.52 ± 1.05 10.45 0.92 0.4 ± 0.1 −32 ± 5
VLA1.1.16 2.779 -0.122 - 49.67 ± 0.21 13.03 1.55 0.5 ± 0.1 −34 ± 5
VLA1.1.17 11.662 7.095 - 5.72 ± 0.04 8.90 1.65
VLA1.1.18 12.673 8.083 - 14.22 ± 0.10 9.29 1.08
VLA1.1.19 16.251 11.299 - 9.16 ± 0.26 11.37 0.97
VLA1.1.20 16.378 10.674 - 13.52 ± 0.02 19.67 1.87 0.7 ± 0.1 −41 ± 5
VLA1.1.21 17.767 13.378 - 8.08 ± 0.25 11.37 0.77
VLA1.1.22 36.250 24.662 - 21.39 ± 0.37 9.79 1.38
VLA1.1.23 36.418 20.989 - 15.00 ± 0.10 12.27 2.05
VLA1.1.24 37.639 20.233 - 62.51 ± 0.14 12.58 0.72 0.6 ± 0.1 −22 ± 4
VLA1.1.25 38.397 21.591 - 680.26 ± 0.61 14.14 1.36 0.6 ± 0.1 −35 ± 2
VLA1.1.26 40.418 21.824 - 134.29 ± 0.25 13.19 0.68 0.5 ± 0.1 −40 ± 4
VLA1.1.27 40.460 22.739 - 42.89 ± 0.24 13.19 0.83 1.3 ± 0.1 −23 ± 2
VLA1.1.28 54.943 31.521 - 3.67 ± 0.13 12.50 0.88

Notes.

a

The reference position is α2000 = 20h38m36s​.43399 ± 0s​.00008 and δ2000 = +42° 37′34″​​.8710 ± 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 ∼ 3600 K (Γν = 19 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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