Fig. 20

Infall velocity field of the envelope of Cha-MMS1 based on the radiative transfer modelling with MAPYSO. The solid black line corresponds to the velocity profile of the “MCS”, “MHCOP”, and “MCO” models. The dashed lines show the range of velocity fields that are still consistent with the observations. The red solid and dashed curves correspond to the average radial velocity at the equatorial plane of a magnetised FHSC with core masses of 1 M⊙ and 5 M⊙, and ages of 850 yr and 2684 yr, respectively. (Commerçon et al. 2012, see details in Sect. 5.4.2).
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