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Table A.5

Observed and fitted properties of the C18O J = 10–9 line profiles for the detected sources.

Source FWHM rmsa
(K km s-1) (K) (km s-1) (mK)

Low-mass: Class 0
NGC 1333 IRAS 2A 0.34 0.04 10.7 8
NGC 1333 IRAS 4B 0.05 0.03 1.4 10
Ser SMM 1 0.61 0.07 4.8 17

Low-mass: Class I
GSS 30 IRS1 0.12 0.04 3.1 8
Elias 29 0.22 0.04 4.7 7

High-mass
IRAS 05358+3543 0.42 0.10 3.8 26
IRAS 16272−4837 0.49 0.11 4.8 26
NGC 6334-I(N) 2.31 0.28 7.5 20
W43-MM1 0.92 0.12 5.3 23
DR21(OH) 7.94 1.08 6.0 33
W3-IRS5 17.04 3.39 4.1 22
IRAS 18089−1732 1.54 0.30 4.5 28
W33A 1.72 0.30 4.3 22
IRAS 18151−1208 0.48 0.09 4.2 22
AFGL2591 3.80 0.88 3.4 23
G327−0.6 3.03 0.42 5.8 34
NGC 6334-I 10.09 1.55 5.3 28
G29.96−0.02 5.79 1.02 4.5 30
G31.41+0.31 3.98 0.52 6.1 38
G5.89−0.39 11.59 2.08 7.0 27
G10.47+0.03 3.44 0.47 7.1 26
G34.26+0.15 11.80 1.73 6.0 29
W51N-e1 10.49 1.48 6.8 52
NGC 7538-IRS1 3.95 0.88 3.9 37

Notes.

(a)

In 0.27 km s-1 bins.

(b)

Integrated over the entire line.

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