Intermediate-mass pre-main-sequence stars exhibit less lithium depletion than lower-mass counterparts overall, with disk-locking effective for roughly half the timescale of lower-mass stars, supporting magnetospheric accretion and a possible pre-main-sequence origin for planet-lithium relations.
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Lithium and the evolution of intermediate-mass T Tauri and Herbig stars. Rotation, accretion, and planets
Intermediate-mass pre-main-sequence stars exhibit less lithium depletion than lower-mass counterparts overall, with disk-locking effective for roughly half the timescale of lower-mass stars, supporting magnetospheric accretion and a possible pre-main-sequence origin for planet-lithium relations.