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Table 1

Ammonia source sample and observing parameters.

Source Stage RA(J2000) Dec(J2000) Lbol M αvir d Tsys tON
(h:m:s) (°::′′) (L) (M) (pc) (K) (min)

G34.41+0.2 IRDC 18:53:18.13 01:25:23.7 4.8(3) 1.5(2) 1.68 1600 1990 11.9
G23.21-0.3 IRDC 18:34:54.91 –08:49:19.2 1.3(4) 1.1(3) 0.57 4600 1600 23.8
G327.29-0.6 HC 15:53:07.80 –54:37:06.4 8.2(4) 2.4(3) 1.72 3100 1960 9.4
G34.26+0.2 UCHII 18:53:18.49 01:14:58.7 4.6(4) 6.8(2) 0.95 1600 1920 18.8
G351.58-0.4 UCHII 17:25:25.03 –36:12:45.3 2.4(5) 7.4(3) 0.42 6800 2020 18.8
G35.20-0.7 MYSO 18:58:12.93 01:40:40.6 2.5(4) 3.8(2) 1.11 2200 1940 18.2
G5.89-0.4 UCHII 18:00:30.40 24:04:00.0 3.6(4) 1.4(2) 1300 1890 12.5
W33A MYSO 18:14:39.52 –17:52:00.5 3.0(4) 7.0(2) 2400 2000 6.2
W49N UCHII 19:10:13.20 09:06:12.0 3.6(6) 3.4(4) 11100 1930 10.7

W43MM1 MYSO Wyrowski et al. (2012) 6.3(4) 4.6(3) 1.12 4900
G31.41+0.31 HC Wyrowski et al. (2012) 6.7(4) 2.7(3) 0.61 4900

Notes. Distances, luminosities, and masses are taken from König et al. (2015) except for G5.89 and W33A, which are taken from van der Tak et al. (2013). Virial parameters are adopted from Giannetti et al. (2014). Additionally, updated parameters for sources from Wyrowski et al. (2012) are listed.

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