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We present the first quantitative results explaining the presence in theLarge Magellanic Cloud of some asymptotic giant branch stars that share theproperties of lithium rich carbon stars. A self-consistent description oftime-dependent mixing, overshooting, and nuclear burning was required. Weidentify a narrow range of masses and luminosities for this peculiar stars.Comparison of these models with the luminosities of the few Li-rich C stars inthe Large Magellanic Cloud provides an independent distance indicator for theLMCComment: 7 pages, 2 figure

Modeling Lithium-rich Carbon Stars in the Large Magellanic Cloud: An Independent Distance Indicator?