The Li overabundance of J37: Diffusion or accretion?

Details The Li overabundance of J37: Diffusion or accretion? The Li overabundance of J37: Diffusion or accretion?

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.560..403a&link_type=gif

Proceedings of the 13th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, held 5-9 July, 2004 in Hamburg, Germany.

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