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Table 2

Summary of the observational parameters of C18O (2–1) spectral line.

Protocluster (name) Spectral resolution (km s−1) Beam major (θmajor) (″) Beam minor (θminor) (″) Position angle (PA) (°) RMS noise (σrms) (mJy beam−1)
W43-MM1 0.17a 0.65 0.49 −80.63 5.0
W43-MM2 0.33 0.79 0.63 −83.67 4.1
G327.29 0.33 0.86 0.79 −55.97 18.6
G328.25 0.33 1.23 1.21 −37.49 29.8
G337.92 0.33 0.70 0.55 −49.02 9.6
G338.93 0.33 0.77 0.70 76.36 8.0
W43-MM3 0.33 0.76 0.67 84.49 4.8
W51-E 0.33 0.42 0.33 29.81 6.3
G008.67 0.33 0.97 0.78 −82.98 15.7
G351.77 0.33 1.14 0.89 88.68 20.0
G353.41 0.33 1.19 0.91 85.55 21.0
W51-IRS2 0.33 0.76 0.68 −26.43 4.5
G010.62 0.33 0.65 0.49 −67.97 12.8
G012.80 0.33 1.33 0.90 77.41 19.0
G333.60 0.33 0.76 0.69 −23.64 8.1

Notes. Col. 1: source name of the protoclusters. Col. 2: spectral resolution of the observations. Col. 3: size of the major axis of the clean beams. Col. 4: size of the minor axis of the clean beams. Col. 5: position angle (PA) of the clean beams. Col. 6: achieved RMS noises of the C18O (2–1) feathered image cubes. a Only for W43-MM1 region, the spectral resolution is 0.17 km s−1, because this data was taken from the pilot project of Motte et al. (2018).

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