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Fig. A.2


Several isochrones of different ages and rotating stellar evolution models are shown in the HR diagram. The surface rotational velocity at the ZAMS is chosen in steps of 100 km s-1 from non-rotating to 400 km s-1 and additionally 450 km s-1. Three initial surface rotational velocities are highlighted in particular. The isochrones of non-rotating models are shown in red, 400 km s-1 in blue, and 450 km s-1 in orange.

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