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Fig. 3

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Maximum central density nc,f attainable for a given evolutionary track compared to the initial nc,i, both plotted as functions of the gravitational mass of the initial non-rotating configuration, Mi. Upper panel: spin-up scenario. The reference line nc,i is the static sequence. Lower panel: spin-down scenario. The reference nc,i line is the mass-shedding limit, to be compared with nc,f of static configurations (DH EOS).

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