Fig. 1

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W43-MM2&MM3 (a) and W43-MM1 (b) protoclusters, as imaged at 1.3 mm by the ALMA 12-m array. The sources extracted with getsf are represented by ellipses showing their size at FWHM. Cores listed in Tables F.1 and F.2 are numbered in cyan for protostellar cores and in white for prestellar cores above the completeness limit (1.6 M⊙ and 0.8 M⊙ in a and b, resp.). bsens and bsens* continuum images are shown in (a) and (b), respectively. Rectangles in cyan in (b) indicate the position of the zooms provided in Fig. E.3 to highlight a new high-mass prestellar core candidate and new core-outflow associations. Ellipses in the lower left corners represent the angular resolution of the image and scale bars indicate the size in physical units.
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