@article {23973,
	title = {Lithium in Large Magellanic Cloud carbon stars},
	volume = {341},
	year = {2003},
	month = {2003/06/1},
	pages = {1290 - 1298},
	abstract = {19 carbon stars that show lithium enrichment in their atmospheres have been discovered among a sample of 674 carbon stars in the Large Magellanic Cloud. Six of the Li-rich carbon stars are of the J type, i.e. they show strong <SUP>13</SUP>C isotopic features. No super-Li-rich carbon stars were found. The incidence of lithium enrichment among carbon stars in the LMC is much rarer than in the Galaxy, and about five times more frequent among J-type than among N-type carbon stars. The bolometric magnitudes of the Li-rich carbon stars range between -3.3 and -5.7. Existing models of Li-enrichment via the hot bottom burning process fail to account for all of the observed properties of the Li-enriched stars studied here.},
	keywords = {Abundances, Astrophysics, Magellanic Clouds, Nuclear Reactions, Nucleosynthesis, Stars: carbon},
	isbn = {0035-8711},
	url = {https://ui.adsabs.harvard.edu/abs/2003MNRAS.341.1290H},
	author = {Hatzidimitriou, D. and Morgan, D. H. and Cannon, R. D. and Croke, B. F. W.}
}
