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Fig. 8


Snapshot of a MHD simulation of a 10 000 M collapsing cloud (see Appendix C for more details; Schneider et al. 2010). a) Column density (colour and contours) smoothed to the resolution of the ALMA data (5′′). The arrows show the plane-of-the-sky velocity field. We see that gas flows along filaments and also off the filaments. b) Dense gas line-of-sight velocity field (colour scale) smoothed to the resolution of the ALMA data. We highlighted the filaments by white dashed lines. The contours are the same as in panel a).

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