X-ray luminosity vs. rotational period for h Per members, with masses ranging between 0.7 and 1.0 M⊙ (green), and 0.3 and 0.7 M⊙ (orange), compared with supersaturation behavior predicted by centrifugal stripping models (dashed gray and black lines are computed assuming that the coronal extends up to 1 R⋆ and 2 R⋆ over the stellar surface).
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