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Table A.2

Observed and fitted properties of the 13CO J = 10–9 line profiles for the detected sources.

Source rmsa b FWH MB FWH MN
(mK) (K km s-1) (K) (K) (km s-1) (km s-1) (km s-1) (km s-1)

Low-mass: Class 0
L 1448-MM 20 0.2 0.1 4.7 1.6
NGC 1333 IRAS 2A 15 0.8 0.2 7.5 2.1
NGC 1333 IRAS 4A 23 1.1 0.07 0.09 5.7 6.7 13.2 0.7
NGC 1333 IRAS 4B 17 0.8 0.1 6.9 6.8
IRAS 15398 24 0.2 0.16 5.0 1.1
BHR 71 17 0.4 0.2 –4.6 1.8
L 483-MM 16 0.3 0.1 5.0 2.4
Ser SMM 1 22 4.0 0.2 0.5 7.6 8.3 10.6 2.4
Ser SMM 3 20 0.3 0.1 7.2 4.0
Ser SMM 4 25 0.6 0.1 5.7 6.0
L 723-MM 16 0.3 0.1 11.5 2.7
B335 20 0.3 0.1 8.1 2.3
L 1157 20 0.1 0.05 3.0 2.2

Low-mass: Class I
L 1489 32 0.4 0.05 7.8 7.3
L 1551 IRS 5 29 1.3 0.47 6.5 2.4
TMR 1 29 0.3 0.08 6.0 3.6
HH 46 30 0.1 0.11 5.4 1.5
IRAS 12496 28 0.8 0.15 3.1 4.2
GSS 30 IRS1 33 2.0 0.46 2.8 3.4
Elias 29 28 2.1 0.38 4.7 5.1

Intermediate-mass
L1641 S3 MMS1 38 1.8 0.2 4.7 6.1
Vela IRS 19 41 1.1 0.2 12.1 5.9
Vela IRS 17 43 4.9 0.8 0.4 4.4
NGC 7129 FIRS 2 20 0.9 0.1 –9.6 4.3
NGC 2071 17 16.6 0.4 2.1 9.1 9.8 14.7 4.7
AFGL 490 47 2.6 0.3 –13.5 4.8

High-mass
IRAS 05358+3543 18 6.2 0.2 0.7 –15.1 –15.9 15.4 3.7
IRAS 16272−4837 18 3.9 0.7 –47.0 4.8
NGC 6334-I(N) 23 13.8 0.5 1.3 –5.7 –3.8 13.3 4.4
W43-MM1 38 4.5 0.8 98.4 5.8
DR21(OH) 18 52.2 0.9 5.7 –1.9 –3.3 16.0 5.8
W3-IRS5 21 129.6 2.1 17.0 –38.7 –38.3 14.7 4.7
IRAS 18089−1732 27 8.3 1.4 33.0 4.6
W33A 19 11.4 0.5 1.1 36.8 37.7 11.7 3.5
IRAS 18151−1208 19 3.4 0.8 33.4 3.6
AFGL2591 19 29.5 0.8 5.4 –5.8 –5.4 9.8 3.3
G327−0.6 25 12.8 1.8 –44.8 6.6
NGC 6334-I 23 57.7 0.7 7.2 –6.7 –6.8 17.8 5.4
G29.96−0.02 46 31.3 0.6 4.6 96.9 98.8 13.6 4.6
G31.41+0.31 52 17.4 2.5 96.8 6.1
G5.89−0.39 34 133.7 2.6 6.2 10.5 9.4 21.9 5.9
G10.47+0.03 200 26.2 1.8 66.8 10.0
G34.26+0.15 59 58.8 1.3 6.7 58.0 57.7 12.0 5.0
W51N-e1 50 70.2 1.3 5.0 58.6 57.1 18.6 7.2
NGC 7538-IRS1 24 41.0 2.0 5.3 –59.8 –57.6 8.7 3.5

Notes.The subscript B refers to the broad velocity component and the N to the narrow component.

(a)

In 0.27 km s-1 bins.

(b)

Integrated over the entire line.

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