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Fig. A.3

image

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. 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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