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Table 3

CORE parameters.

Source Beam Lin. res.d uv-radiuse rms rmssc 5σ Speak Sint mfa T(H2CO) Δv(H2CO)
(″, PA) (AU) (m) (mJy beam−1) (mJy beam−1) (M) (mJy beam−1) (mJy) (%) (K) (km s−1)
IRAS 23151 0.45″ × 0.37″(50°) 1350 21-764 0.19 0.10 0.05 32.6 100 78 59 3.4
IRAS 23033 0.45″ × 0.37″(47°) 1760 20-765 0.46 0.28 0.28 38.9 310 64 55 3.5
AFGL2591 0.47″ × 0.36″(65°) 1370 31-765 0.60 0.40 0.18 87.3 249 84 69 3.1
G75.78 0.48″ × 0.37″(60°) 1615 21-765 0.60 0.42 0.16 64.7 256 87 108 5.3
S87IRS1 0.54″ × 0.35″(37°) 980 16-765 0.23 0.21 0.06 33.7 214 87 48 3.7
S106 0.47″ × 0.34″(47°) 530 19-765 1.25 0.62 0.02 73.9 170 87 135 4.8
IRAS 21078 0.48″ × 0.33″(41°) 650 34-765 0.60 0.28 0.03 34.7 1020 53 66 4.9
G100 0.49″ × 0.33″(56°) 1440 16-765 0.08 0.05 0.03 8.5 67 b 58 2.3
G084 0.43″ × 0.38″(69°) 2230 15-753 0.10 0.08 0.22 6.2 85 67c 35 3.5
G094 0.41″ × 0.39″(77°) 1600 15-762 0.14 0.11 0.36 13.6 90 81 18 2.5
CepA 0.44″ × 0.38″(80°) 290 19-765 4.00 1.70 0.02 440.9 1225 72 119 5.3
NGC 7538IRS9 0.44″ × 0.38″(80°) 1110 19-765 0.30 0.15 0.04 41.2 237 76 86 4.0
W3(H2O) 0.43″ × 0.32″(86°) 750 19-760 4.50 1.90 0.13 451.6 5292 25 162 6.6
W3IRS 4 0.45″ × 0.32″(83°) 770 19-762 0.60 0.60 0.11 39.3 377 87 66 4.2
G108 0.50″ × 0.44″(49°) 2020 17-765 0.25 0.15 0.24 14.8 60 b 36 3.3
IRAS 23385 0.48″ × 0.43″(58°) 2230 18-764 0.25 0.11 0.11 18.0 190 56 73 3.8
G138 0.50″ × 0.41″(60°) 1320 20-764 0.16 0.16 0.12 6.2 100 82 36 2.9
G139 0.51″ × 0.40″(56°) 1460 21-764 0.17 0.15 0.10 13.9 26 95 48 1.4

Previous pilot study
NGC 7538IRS1 0.33″ × 0.32″(-55°) 880 68-765 10.0 5.20 1.34 2334 2838 50 82 4.5
NGC 7538S 0.34″ × 0.31″(-81°) 880 68-765 0.60 0.50 0.14 28.1 253 91 78 5.6

Notes. The columns give the synthesized beam, the linear resolution, the baseline range (uv-radius), the rms noise before and after self-calibration, the 5σ mass sensitivity, the measured peak, and integrated flux densities Speak and Sint, the missing flux ratios as well as the H2CO derived temperatures T and line widths Δv. (a) Missing flux, for details see main text, (b) no single-dish data available, (c) based on BOLOCAM 1.1 mm flux measurement in 40″ aperture (Ginsburg et al. 2013), (d)average linear resolution, (e)projected uv baseline range.

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