Fig. 5
Velocity profiles at t = 16 tdyn for the different runs. Left panel: A1 (blue solid), A1_t (green dashed), A1_t_nw (red dotted), I1 (cyan solid), I1_t (purple dashed), I1_t_nw (black dotted), and IrrI1_t (yellow solid); middle panel: A2 (blue solid), A2_t (green dashed), A2_t_nw (red dotted), I2 (cyan solid), I2_t (purple dashed), I2_t_nw (black dotted), and IrrI2_t (yellow solid); right panel: A3 (blue solid), A3_t (green dashed), A3_t_nw (red dotted), I3 (cyan solid), I3_t (purple dashed), I3_t_nw (black dotted), and IrrI3_t (yellow solid). The black solid line corresponds to the Keplerian velocity
for a star with mass M = 2.5 M⊙.
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