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Table 1

Parameters of the 6.7-GHz CH3OH maser features detected in IRAS 20126+4104.

     (1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
Maser Group RAa Deca Peak flux V lsr ΔvL P l b χ b ΔVi c TBΔΩ c P V ΔVZ θ d
offset offset density(I)
(mas) (mas) (Jy/beam) (km s-1) (km s-1) (%) (°) (km s-1) (log K sr) (%) (m s-1) (°)

M01 2 14.869 5.734 0.917    ±    0.003 6.72 0.29
M02 2 11.405 3.063 0.964    ±    0.003 6.72 0.36
M03 2 2.797 19.127 0.265    ±    0.009 6.10 0.20
M04 2 1.743 16.438 0.275    ±    0.007 5.97 0.25
M05 2 0 0 27.838    ±    0.009 6.10 0.36 1.6    ±    0.4 -9.2    ±    1.4
M06 2 0.129 7.450 0.316    ±    0.007 6.14 0.30
M07 2 0.947 8.122 0.543    ±    0.008 6.01 0.31
M08 2 9.382 4.685 0.428    ±    0.007 5.97 0.25
M09 2 19.883 7.031 0.199    ±    0.007 6.23 0.20
M10 2 19.904 11.261 0.049    ±    0.003 5.66 0.23
M11 2 52.634 48.145 0.068    ±    0.002 5.13 0.28
M12 2 56.313 21.915 0.308    ±    0.002 5.57 0.38
M13 2 62.231 15.331 0.861    ±    0.003 6.41 0.27
M14 2 81.877 10.986 0.919    ±    0.003 6.67 0.28
M15 83.835 244.766 0.070    ±    0.003 6.50 0.19
M16 1 166.917 77.072 0.048    ±    0.002 5.18 0.19
M17 1 155.448 104.588 0.178    ±    0.002 4.87 0.23
M18 1 191.556 37.796 1.851    ±    0.003 7.64 0.27 1.4    ±    0.1 71    ±    5
M19 1 192.782 25.593 0.117    ±    0.003 7.68 0.23
M20 1 204.295 7.683 0.309    ±    0.003 7.11 0.21
M21 1 207.436 33.264 0.072    ±    0.003 7.51 0.19
M22 1 210.965 16.399 0.114    ±    0.003 6.50 0.21
M23 1 215.312 8.267 0.402    ±    0.003 6.98 0.36
M24 1 237.153 4.383 2.154    ±    0.003 6.98 0.30 0.6    ±    0.2 56    ±    43
M25 1 261.232 4.707 0.166    ±    0.003 7.72 0.28
M26 1 277.392 3.834 0.644    ±    0.002 8.25 0.26

Notes.

(a)

The reference position is and (see Sect. 4).

(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 by 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. 2011a). The errors were determined by analyzing the full probability distribution function.

(d)

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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