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Table A.3

Observed and fitted properties of the H2O 211–202 line for the detected intermediate- and high-mass YSOs.

Source rmsa b FWZI
(mK) (K) (K km s-1) (km s-1)

Inter.-mass
NGC 7129 FIRS2 22 0.52 7.76 ± 0.02 48
L1641 S3MMS1 28 0.24 2.69 ± 0.05 22
NGC 2071 37 3.78 62.30 ± 0.04 123
Vela IRS17 30 0.82 8.13 ± 0.03 39
Vela IRS19 36 0.41 3.74 ± 0.04 63
AFGL490 100 0.51 22.46 ± 0.03 33
OMC-2-FIR 4 15 1.87 29.92 ± 0.05 69

High-mass
IRAS 05358+3543 44 2.01 27.57 ± 0.05 100
IRAS 16272-4837 81 2.37 21.70 ± 0.08 60
NGC 6334I-N-1 92 4.38 117.17 ± 0.17 90
W43-MM1 48 2.77 45.14 ± 0.05 108
DR21-OH 68 7.48 104.18 ± 0.07 90
W3-IRS5 68 9.09 112.14 ± 0.07 105
IRAS 18089-1732 68 1.72 15.62 ± 0.07 36
W33A 79 2.76 30.17 ± 0.08 60
IRAS 18151-1208 36 0.86 6.41 ± 0.04 40
AFGL2591 37 3.76 21.37 ± 0.04 42
G327-0.6 147 5.19 60.08 ± 0.15 66
NGC 6334-I-1 152 9.69 78.44 ± 0.06 117
G29.96-0.02 96 4.05 42.21 ± 0.10 69
G31.41+0.31 74 2.28 23.93 ± 0.08 57
G5.89-0.39 59 10.67 285.22 ± 0.06 144
G10.47+0.03 73 4.47 45.81 ± 0.07 27
G34.26+0.15 225 10.24 93.03 ± 0.10 42
W51N-e1 242 9.46 150.81 ± 0.24 42
NGC 7538-IRS1 61 6.97 49.10 ± 0.06 42

Notes. FWZI has been calculated by binning the spectra to 3 km s-1.

(a)

In 0.27 km s-1 bin.

(b)

Integrated over the interval of velocities defined by the FWZI.

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