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).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.