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Fig. C.12

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Collapse of a gaseous sphere followed by star formation and protostellar accretion. The top panel shows the radial distributions of the gas number density at different time instances during the collapse and after the formation of the star. The red line is the fit to Eq. (C.12) with A = 5. The bottom panel displays the resulting mass accretion on to the star. The time is counted from the onset of simulations.

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