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Fig. A.1
Radial profiles of the density, velocity, and the ratio of gas to ram pressure for collapse of a 1 M⊙ cloud for three different cases, using an initial Bonnor–Ebert sphere (blue) at 10 K, uniform cloud at 10 K (dashed red), and uniform cloud at 30 K (dashed yellow) are shown at a time step after the second core formation.
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