The evolution of lithium in FGK dwarf stars: The Li rotation connection and the Li desert
F. Llorente de Andr\'es, C. Chavero, R. de la Reza, S. Roca-F\`abrega, and C. Cifuentes

TL;DR
This study explores the lithium-rotation connection and the lithium desert in FGK dwarf stars, revealing age-dependent lithium depletion linked to stellar rotation and suggesting the lithium desert may be a statistical artifact rather than a distinct feature.
Contribution
It provides the first analysis of the lithium rotation connection across stellar associations aged 45-120 Myr and questions the reality of the lithium desert as a distinct phenomenon.
Findings
Critical rotation velocity separating slow and rapid rotators is 5 km/s.
Minimum lithium depletion varies with age, decreasing from ~50 km/s to less than 20 km/s over 200 Myr.
The lithium desert may be a statistical fluctuation, not a real feature.
Abstract
We investigate two topics regarding solar mass FGK-type stars, the lithium rotation connection (LRC) and the existence of the "lithium desert". We determine the minimum critical rotation velocity () related with the LRC separating slow from rapid stellar rotators, as being 5 km s. This value also split different stellar properties. For the first time we explore the behaviour of the LRC for some stellar associations with ages between 45 Myr and 120 Myr. This allows us to study the LRC age dependence at the beginning of the general spin down stage for low mass stars, which starts at 30-40 Myr. We find that each stellar group presents a characteristic minimum lithium (Li) depletion connected to a specific large rotation velocity and that this minimum changes with age. For instance, this minimum changes from 50 km s to less than 20 km s in 200…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Solar and Space Plasma Dynamics
