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J.R. King, S.C. Schuler (Clemson University)
Recent evidence has suggested that some portion of the scatter in star-to-star Li abundances as well as the Li-Teff relation in open cluster dwarfs may be spuriously caused by NLTE effects. Using new and extant literature data, we explore the relation between abundances and chromospheric emission in solar-type stars in several open clusters. This work is supported by NSF grant AST-0086576 to JRK.
The author(s) of this abstract have provided an email address for comments about the abstract: jking2@ces.clemson.edu
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Bulletin of the American Astronomical Society, 35 #3
© 2003. The American Astronomical Soceity.