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Table A.2

Observed and fitted properties of the H2O 202–111 line for the detected intermediate- and high-mass sources.

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

Inter.-mass
NGC 7129 FIRS2 18 0.58 9.50 ± 0.02 48
L1641 S3MMS1 23 0.30 6.28 ± 0.03 48
NGC 2071 38 3.83 76.98 ± 0.04 108
Vela IRS17 22 0.74 9.97 ± 0.02 63
Vela IRS19 21 0.34 6.23 ± 0.02 72
AFGL490 21 0.44 6.94 ± 0.02 75
OMC-2-FIR 4 28 3.15 52.31± 0.04 66

High-mass
IRAS 05358+3543 57 1.93 24.69 ± 0.09 54
IRAS 16272-4837 81 1.34 17.34 ± 0.11 39
NGC 6334I-N-1 60 2.25 43.55 ± 0.09 57
W43-MM1 54 1.02 25.99 ± 0.06 84
DR21-OH 73 5.86 29.39 ± 0.11 51
W3-IRS5 95 7.07 88.32 ± 0.12 63
IRAS 18089-1732 107 1.27 12.01 ± 0.14 27
W33A 47 2.23 24.13 ± 0.05 63
IRAS 18151-1208 96 0.82 4.88 ± 0.12 30
AFGL2591 100 3.41 17.21 ± 0.13 24
G327-0.6 91 3.23 33.50 ± 0.14 51
NGC 6334-I-1 106 5.32 69.44 ± 0.14 60
G29.96-0.02 67 5.36 62.34 ± 0.07 66
G31.41+0.31 61 1.41 18.74 ± 0.07 60
G5.89-0.39 67 9.60 265.34 ± 0.07 108
G10.47+0.03 104 3.58 34.75 ± 0.12 39
G34.26+0.15 64 6.08 48.49 ± 0.07 60
W51N-e1 64 6.75 102.12 ± 0.07 81
NGC 7538-IRS1 91 5.56 37.20 ± 0.12 24

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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