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Table 1

15 massive protoclusters targeted by ALMA-IMF.

Field Cube center [IRCS - J2000] VLSR d Evolutionary Mcloud
RA[h:m:s] Dec[°:′:″] [km s−1] [kpc] stage [× 103 M]
G008.67 18:06:21.12 −21:37:16.7 +37.6 3.4 I 3.1
G010.62 18:10:28.80 −19:55:48.3 −2.0 5.0 E 6.7
G012.80 18:14:13.37 −17:55:45.2 +37.0 2.4 E 4.6
G327.29 15:53:08.13 −54:37:08.6 −45.0 2.5 Y 5.1
G328.25 15:57:59.68 −53:57:59.8 −43.0 2.5 Y 2.5
G333.60 16:22:09.36 −50:05:59.2 −47.0 4.2 E 12.0
G337.92 16:41:10.62 −47:08:02.9 −40.0 2.7 Y 2.5
G338.93 16:40:34.42 −45:41:40.6 −62.0 3.9 Y 7.1
G351.77 17:26:42.62 −36:09:20.5 −3.0 2.0 I 2.5
G353.41 17:30:26.28 −34:41:49.7 −17.0 2.0 I 2.5
W43-MM1 18:47:47.00 −01:54:26.0 +97.0 5.5 Y 13.4
W43-MM2 18:47:36.61 −02:00:51.7 +97.0 5.5 Y 11.6
W43-MM3 18:47:41.46 −02:00:28.2 +97.0 5.5 I 5.2
W51-E 19:23:44.18 +14:30:28.9 +55.0 5.4 I 32.7
W51-IRS2 19:23:39.81 +14:31:02.9 +55.0 5.4 E 20.6

Notes. The central positions of the mosaics are taken from the CH3OCHO cube headers. The rest velocities (VLSR), distances to the Sun (d), evolutionary stages (Young, Intermediate, Evolved), and cloud mass (Mcloud) computed from the 870 μm integrated flux, are from Paper I.

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