Binary mass transfer from intermediate-mass AGB stars can explain the most lithium-rich giants, with preferred separations near 3.3 AU and low mass transfer efficiency.
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Probing Binary Architectures of Lithium-Rich Giants in GALAH with COSMIC and Stellar Models
Binary mass transfer from intermediate-mass AGB stars can explain the most lithium-rich giants, with preferred separations near 3.3 AU and low mass transfer efficiency.