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Table 2

All 6.7-GHz methanol maser features detected in W51–IRS2.

     (1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
Maser RAa Deca Peak flux Vlsr ΔvL Pl χ ΔVib TbΔΩb ΔVZc θd
offset offset density(#I)
(mas) (mas) (Jy/beam) (km s-1) (km s-1) (%) (°) (km s-1) (log K sr) (m/s) (°)

W51N.01 –85.860 –28.289 0.27 ± 0.01 54.52 0.31  −  −  −  −  −  −
W51N.02 –83.367 –22.108 0.20 ± 0.01 54.96 0.28  −  −  −  −  −  −
W51N.03 –53.067 –11.479 0.33 ± 0.04 57.94 0.28  −  −  −  −  −  −
W51N.04 –45.312 8.416 0.90 ± 0.02 57.51 0.25  −  −  −  −  −  −
W51N.05 –33.569 –351.122 0.61 ± 0.02 59.70 0.18  −  −  −  −  −  −
W51N.06 –25.536 –312.023 0.47 ± 0.03 59.88 0.28  −  −  −  −  −  −
W51N.07 –12.962 13.928 0.74 ± 0.02 55.84 0.25  −  −  −  −  −  −
W51N.08 –9.140 –108.629 1.02 ± 0.03 56.28 0.29  −  −  −  −  −  −
W51N.09 –6.813 –2.965 1.93 ± 0.01 56.45 0.21  −  −  −  −  −  −
W51N.10 –5.152 –16.856 1.12 ± 0.03 56.28 0.35  −  −  −  −  −  −
W51N.11 0 0 12.03 ± 0.07 56.19 0.35 1.3 ± 1.1 27 ± 13  −
W51N.12 1.496 18.406 0.95 ± 0.01 56.63 0.36  −  −  −  −  −  −
W51N.13 5.096 –6.713 1.25 ± 0.01 55.75 0.30  −  −  −  −  −  −
W51N.14 5.373 –161.138 2.42 ± 0.05 59.79 0.24  −  −  −  −  −  −
W51N.15 10.192 6.065 0.57 ± 0.01 56.98 0.31  −  −  −  −  −  −
W51N.16 12.630 –129.178 0.48 ± 0.02 60.84 0.26  −  −  −  −  −  −
W51N.17 24.761 –149.938 0.16 ± 0.01 60.23 0.26  −  −  −  −  −  −
W51N.18 64.644 26.281 0.20 ± 0.02 55.75 0.28  −  −  −  −  −  −

Notes. 

(a)

The reference position is α2000 = 19h23m39s.818 and .

(b)

The best-fitting results obtained by using a model based on the radiative transfer theory of methanol masers for Γ + Γν = 1 (Vlemmings et al. 2010; Surcis et al. 2011b). The errors were determined by analyzing the full probability distribution function.

(c)

The Zeeman-splittings are determined from the cross-correlation between the RR and LL spectra.

(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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