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Table 6:

Comparison of masses derived from p-ArTéMiS 450 $\mu $m and ATCA NH3 (1,1) emission.
Clump RA Dec Mass Mass [NH3] / [H2]$^{\alpha }$ Average Aliases
ID (J2000) (J2000) 450 $\mu $m NH3 LTE Abundance $T_{\rm dust}$ (André et al. 2008)
      ($M_{\odot}$) ($M_{\odot}$)      

S1-a
11:12:21.09 -61:17:09.50 89 91 $3.1\times10^{-8}$ 15 -
S1-b 11:12:17.21 -61:17:43.50 161 140 $2.6\times10^{-8}$ 21 S1-M1
S1-c 11:12:14.43 -61:17:17.50 193 82 $1.3\times10^{-8}$ 23 S1-M2
S3-a 11:11:53.05 -61:18:31.37 357   51 $0.4\times10^{-8}$ 40 S3-M4
S3-b 11:11:45.54 -61:18:45.27 682 211 $0.9\times10^{-8}$ 38 S3-C3
S4-a 11:11:39.69 -61:19:43.18 161 383 $7.1\times10^{-8}$ 24 S4-M6
S4-b 11:11:36.91 -61:20:03.13 247 279 $3.4\times10^{-8}$ 19 -
S5 11:11:34.66 -61:21:11.09 712 339 $1.4\times10^{-8}$ 15 S5-M8

$^{\alpha }$ Relative abundance of NH3 to H2 via a direct comparison of clump masses derived from NH3 and 450  $\mu $m emission.


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