Fig. 2
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Slices of 10 000 AU of three forces ratios when M = 10 M⊙ (L = 2 × 104 L⊙) in run NOTURB (top) and when M = 23.8 M⊙ (L = 1.2 × 105 L⊙) in run LRNOTURB. Left panels: Lorentz against gravitational acceleration. Middle panels: Lorentz acceleration against radiative acceleration. Right panels: radiative acceleration against gravitational acceleration. Lorentz acceleration dominates over the radiative acceleration everywhere but close to the protostar.
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