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Fig. 2.
Evolution of Ṁ⋆ as function of time in case of fast (blue) and slow (red) initially rotating stars. For each rotators, two initial mass accretion rates are investigated Ṁacc = 10−10 (upper panel) and 10−7 (lower panel) M⊙ yr−1 with Qacc = 1 (dotted) and 10% (solid).
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