Signatures of magnetic braking in Class 0 protostars: Exploring the gas kinematics in magnetized models of low-mass star formation

Open Access

Fig. 3

Maps of the azimuthally averaged SAM in the models, $j_{V φ}^{model}$ $j_{V\varphi }^{{\rm{model}}}$ . The white star and dashed blue line depict the location of the protostar and the equatorial plane, respectively. The leftmost panels, from (a) to (f), show the nonturbulent models, while the rightmost panels, from (g) to (k), present the turbulent models’ outputs.

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