Rotation, inflation, and lithium in the Pleiades
Garrett Somers, Marc H. Pinsonneault

TL;DR
This paper presents a physical model linking stellar rotation, radius inflation, and lithium abundance in Pleiades stars, explaining observed correlations through rotationally induced mixing and radius inflation effects.
Contribution
It introduces the first consistent physical model that explains the lithium-rotation correlation in the Pleiades by connecting radius inflation and rotational mixing.
Findings
Radius inflation suppresses lithium destruction in pre-MS stars.
The model reproduces the observed Li-rotation pattern in the Pleiades.
Different inflation prescriptions produce similar qualitative patterns.
Abstract
The rapidly rotating cool dwarfs of the Pleiades are rich in lithium relative to their slowly rotating counterparts. Motivated by observations of inflated radii in young, active stars, and by calculations showing that radius inflation inhibits pre-main sequence (pre-MS) Li destruction, we test whether this pattern could arise from a connection between stellar rotation rate and radius inflation on the pre-MS. We demonstrate that pre-MS radius inflation can efficiently suppress lithium destruction by rotationally induced mixing in evolutionary models, and that the net effect of inflation and rotational mixing is a pattern where rotation correlates with lithium abundance for , and anti-correlates with lithium abundance for , similar to the empirical trend in the Pleiades. Next, we adopt different prescriptions for the dependence of…
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