A search for radius inflation among active M-dwarfs in Praesepe
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DOI: 10.1093/mnras/sty3184
Abstract: Rotation periods from Kepler K2 are combined with projected rotation velocities from the WIYN 3.5-m telescope, to determine projected radii for fast-rotating, low-mass ($0.15 \leq M/M_{\odot} \leq 0.6$) members of the Praesepe cluster. A maximum… read more here.
Keywords: inflation among; radius; radius inflation; among active ... See more keywords