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Fig. 6

image

Ratio of the core-to-surface rotation rate as a function of gravity for models that include magnetic braking of the stellar surface (with a solar-calibrated value for the braking constant). Black, blue, and red continuous lines correspond to an initial velocity on the ZAMS of 50 km s-1 and an additional viscosity of 3 × 104, 1 × 104, and 4 × 103 cm2 s-1, respectively. The green line corresponds to a similar model with an initial velocity on the ZAMS of 10 km s-1 and νadd = 4 × 103 cm2 s-1. The dotted blue line corresponds to a model without surface magnetic braking, with νadd = 1 × 104 cm2 s-1 and an initial velocity on the ZAMS of 8 km s-1. Red dashed vertical lines indicate the values of the gravity of KIC 7341231, while the blue region indicates the lower limit of the core-to-surface rotation rate determined for KIC 7341231.

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