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Fig. 6


Thermal evolution at the centre of the collapsing cloud: the central temperature as a function of the central density for the grey (solid black) and multigroup (solid red) simulations. The different phases of the protostellar collapse are labelled. The results from MI00 (dashed green), Whitehouse & Bate (2006) (dashed purple), SWBG07 (dashed cyan), and Tea13 (dashed blue) are also plotted for comparison. The orange solid line is a grey simulation using an ideal gas EOS.

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