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Table 2

Observed properties of the H2O line profiles.

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

L1448-MM 12 0.32 18.7 138
NGC 1333-IRAS2A 12 0.31 5.2 58
NGC 1333-IRAS4A 12 0.90 17.4 84
NGC 1333-IRAS4B 12 0.69 10.6 54
L1527 10 0.14 1.2 22
Ced110-IRS4 8 0.03 0.3 11
BHR71 12 0.44 10.2 131
IRAS 15398 8 0.21 2.0 28
L483 12 0.14 3.2 22
Ser SMM1 12 0.58 10.8 69
Ser SMM4 12 0.47 8.8 80
Ser SMM3 12 0.13 3.6 80
L723 11 0.13 0.7 15
B335 13 0.09 1.1 26
L1157 13 0.17 3.0 67

NGC 1333-IRAS3 11 0.20 5.2 54
L1489 11 0.08 0.8 41
L1551-IRS5 9 0.12 0.7 19
TMR1 8 0.04 0.3 9
TMC1A 8 0.04 <0.1 ...
TMC1 11 0.05 0.5 19
HH46-IRS 8 0.15 1.2 24
IRAS 12496 8 0.08 0.6 24
GSS30-IRS1d 10 0.72 4.4 35
Elias29 10 0.14 2.0 28
Oph-IRS63 10 0.02 0.1 5
RNO91 10 0.16 0.5 13
RCrA-IRS5A 17 0.50 3.8 34
HH100-IRS 16 0.63 5.3 28

Notes. 

(a)

Measured in 0.3 km s-1 bins.

(b)

Integrated over the entire line, including bullet emission.

(c)

Spectra smoothed to 2 km s-1 resolution and line width measured at the 4-σ level.

(d)

Possible contamination from the VLA1623 outflow.

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