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Table 1

High-mass star-forming regions observed with the VLA.

RA (J2000) Dec (J2000) d(a) M (a) C band(b) K band(b)


Region (h:m:s) (°:′:′′) (kpc) (M) θbeam, PA rms θbeam, PA rms
IRAS 05358+3543 05:39:12.2 +35:45:52.0 1.8 127 1.27 × 1.23, +61 8.1 (c)
G189.78+0.34 06:08:34.5 +20:38:51.0 1.8 150 1.28 × 1.09, +23 16.0 (c)
G192.58−0.04 06:12:52.9 +18:00:34.9 2.6 500 1.40 × 1.19, +21 23.6 (c)
G192.60−0.05 06:12:54.0 +17:59:23.0 2.6 460 1.36 × 1.14, +20 26.5 (c)
G18.18−0.30 18:25:07.3 −13:14:22.9 2.6 110 1.74 × 1.05, −16 10.0 0.54 × 0.31, +25 16.7
IRAS 18223−1243 18:25:10.9 −12:42:27.0 3.7 980 1.89 × 1.14, −14 24.5 0.58 × 0.34, +37 15.0
IRAS 18228−1312 18:25:42.3 −13:10:18.0 3.0 740 1.88 × 1.16, −14 35.0 0.73 × 0.67, −07 59.1
G19.27+0.1M2 18:25:52.6 −12:04:47.9 2.4 114 2.08 × 1.14, −14 9.8 0.50 × 0.32, −26 20.7
G19.27+0.1M1 18:25:58.5 −12:03:58.9 2.4 113 1.95 × 1.19, −16 9.6 0.79 × 0.42, +49 20.0
IRAS 18236−1205 18:26:25.4 −12:03:50.9 2.7 780 1.99 × 1.11, −18 10.2 0.51 × 0.32, −26 16.9
G23.60+0.0M1 18:34:11.6 −08:19:05.9 2.5 365 1.85 × 1.13, −22 8.7 0.54 × 0.30, +32 36.1
IRAS 18316−0602 18:34:20.5 −05:59:30.0 3.1 1000 1.71 × 1.09, −21 8.4 0.53 × 0.30, +35 40.0
G24.08+0.0M2 18:34:51.1 −07:45:32.0 2.5 201 1.80 × 1.13, −21 17.0 0.53 × 0.30, +32 37.0
G24.33+0.1M1 18:35:07.8 −07:35:04.0 3.8 1759 1.69 × 1.25, −13 21.0 0.49 × 0.31, −31 26.1
G24.60+0.1M2 18:35:35.7 −07:18:08.9 3.7 483 1.66 × 1.03, −20 18.2 0.79 × 0.41, +51 21.8
G24.60+0.1M1 18:35:40.2 −07:18:37.0 3.7 192 1.67 × 1.22, −10 12.7 0.75 × 0.38, +57 22.5
G34.43+0.2M3 18:53:20.3 +01:28:23.0 2.5 301 1.57 × 1.46, −59 17.9 0.53 × 0.29, +40 19.0
IRAS 19095+0930 19:11:54.0 +09:35:52.0 3.0 500 1.61 × 1.37, −83 17.0 0.53 × 0.29, +44 63.4

Notes. (a) Distances (d) and clump masses (M) from López-Sepulcre et al. (2011) and Sánchez-Monge et al. (2013b). (b) Synthesized beam (θbeam) major and minor axis in arcsecond, and position angle (PA) in degrees. The rms noise level is given in units of μJy beam−1. Regions marked with and in the first column indicate IR-loud and IR-dark sources, respectively, based on the classification of López-Sepulcre et al. (2010). (c) Region not observed in the K band.

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