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Table 1

Source properties.

Source Da νLSRb Lbolc Tbolc Menvd
(pc) ( km s-1) (L) (K) (M)

IRAS4A 235 +7.2 9.1 33 5.2
L1527 140 +5.9 1.9 44 0.9
BHR71 200 −4.4 14.8 44 3.1
IRAS 15398 130 +5.1 1.6 52 0.5
GSS30-IRS1 125 +3.5 13.9 142 0.6
Ser SMM4 415 +8.0 6.2 26 6.9
L1157 325 +2.6 4.7 46 1.5

Notes.

(a)

Taken from van Dishoeck et al. (2011) with the exception of Ser SMM4, where we use the distance determined using VLBA observations by Dzib et al. (2010).

(b)

Obtained from ground-based C18O or C17O observations (Yıldız et al. 2013b) with the exception of IRAS4A for which the value from Kristensen et al. (2012) is more consistent with our data.

(c)

Measured using Herschel-PACS data from the WISH and DIGIT key programmes (Karska et al. 2013).

(d)

Mass within the 10 K radius, determined by Kristensen et al. (2012) from DUSTY modelling of the sources.

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