Open Access

Fig. 12

image

Survival and disruption regions for stars of mass 0.7, 0.8, 0.9, and 1.1 M. Each row corresponds to a given stellar mass, each column to a given initial stellar rotation. Slow, median, and fast rotators correspond respectively to the 25th, 50th, and 90th percentiles of stellar rotation distributions observed in open clusters as defined by Gallet & Bouvier (2015). For each panel, the orange area represents the region of the (mp,   aini) plane where planets are eventually destroyed, and the blue area the region where planets survive.

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