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Table 1

Properties of the five target clumps in W43-main.

Source RA Dec Gas mass(a) Luminosity(a) L/M Category VLSR(b)
(J2000) (J2000) (102 M) (103 L) (L/M) km s−1
MM2 18h47m36.86 −02º00′49 s.8 38 58 15 70 µm bright 91.3
MM3 18h47m41s.61 −02º00′29 s.5 19 51 26 UCHII 93.9
F1 18h47m42s.77 −01º59′ 42 s.4 3.0 6.6 22 IR dark 89.5
F2 18h47m27s82 −02º01′ 23 s.5 2.3 43 19 IR dark 85.5
C 18h47m42s77 −01º59′ 42 s.4 7.6 12 16 IR dark 91.7

Notes. (a) Gas mass and luminosity are calculated above column density thresholds Nthres: for MM2, MM3 and C, Nthres= 5×1022 cm−2, for F1, Nthres = 4.5×1022 cm−2, for F2, Nthres = 2.2×1022 cm−2; the thresholds are chosen based on visual inspection of the N(H2) and bolometric luminosity maps (derived from integrating SED profile in a pixel-by-pixel basis) from Lin et al. (2016). (b)The system velocities (VLSR) are with reference to Urquhart et al. (2018) based on finding the identical or nearest clumps.

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