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Table A.1

Parameters of the 6.7-GHz CH3OH maser features detected in G30.70-0.07.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
Maser RAa Deca Peak flux Vlsr ΔvL χb TbΔΩc PV ΔVZ |B||| θd
offset offset Density(I)
(mas) (mas) (Jy/beam) (km/s) (km/s) (%) (°) (km/s) (log K sr) (%) (m/s) (mG) (°)
G307.E01 -709.951 427.432 0.565 ± 0.007 87.69 1.03
G307.E02 -707.378 386.938 0.070 ± 0.007 87.73 0.29
G307.E03 -706.234 318.524 0.075 ± 0.005 87.30 0.42
G307.E04 -694.283 547.577 0.309 ± 0.007 86.11 0.41
G307.E05 -687.992 417.643 3.709 ± 0.007 86.15 0.47 1.2 ± 0.1 + 57 ± 5
G307.E06 -685.190 376.825 0.588 ± 0.007 86.11 0.41
G307.E07 -682.674 434.138 0.125 ± 0.032 86.20 0.35
G307.E08 -273.516 13.481 0.730 ± 0.007 89.10 0.26
G307.E09 -271.000 -25.930 0.078 ± 0.007 89.10 0.18
G307.E10 -42.431 95.012 0.132 ± 0.004 89.49 0.45
G307.E11 -36.884 -94.384 0.075 ± 0.003 89.71 0.20
G307.E12 -13.210 -97.353 0.066 ± 0.006 87.38 0.20
G307.E13 -12.409 -93.733 0.068 ± 0.003 90.37 0.28
G307.E14 -4.518 -176.004 0.075 ± 0.009 88.79 1.56
G307.E15 -3.431 -64.735 1.104 ± 0.011 88.44 0.29
G307.E16 -2.745 -62.480 0.347 ± 0.020 88.13 0.30
G307.E17 -1.716 46.170 0.553 ± 0.010 88.09 0.26
G307.E18 -0.114 -0.262 38.158 ± 0.018 88.31 0.30 0.09 ± 0.06 + 49 ± 18 0.7 + 1.5 ± 0.2 > 30
G307.E19 0 0 39.587 ± 0.042 88.31 0.29 0.07 ± 0.02 + 87 ± 18
G307.E20 1.773 -43.808 0.434 ± 0.010 88.09 0.13
G307.E21 3.889 65.256 0.539 ± 0.014 88.13 0.76
G307.E22 4.003 61.158 1.056 ± 0.029 88.57 0.36
G307.E23 5.433 60.280 0.952 ± 0.009 88.57 0.36
G307.E24 6.119 -170.896 0.112 ± 0.013 88.22 0.80
G307.E25 6.748 -412.904 0.101 ± 0.018 88.57 0.13
G307.E26 6.862 -413.448 0.104 ± 0.028 88.57 0.14
G307.E27 11.609 333.790 0.103 ± 0.007 88.31 0.72
G307.E28 19.672 91.844 0.070 ± 0.006 88.31 0.20
G307.E29 127.866 342.210 0.056 ± 0.003 89.32 0.23
G307.E30 127.923 398.027 0.085 ± 0.005 88.96 0.24
G307.E31 266.024 -42.141 0.052 ± 0.004 90.72 0.23

Notes. (a)The reference position is α2000 = 18h47m36s.900 and δ2000 = −02°01′05″.025 (see Sec. 3). (b)Pl and χ are the mean values of the linear polarization fraction and the linear polarization angle measured across the spectrum, respectively. (c)The best-fitting results obtained using a model based on the radiative transfer theory of methanol masers for Γ + Γν = 1 s-1 (Vlemmings et al. 2010; Surcis et al. 2011b). The errors were determined by analyzing the full PDF. (d)The angle between the magnetic field and the maser propagation direction is determined using the observed Pl and the fitted emerging brightness temperature. The errors were determined by analyzing the full PDF. The boldface indicates that |θ+ − 55°| < |θ− 55°|, i.e., the magnetic field is parallel to the linear polarization vector (see Sect. 4).

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