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A. Steinhauer, C. P. Deliyannis (Indiana University)
We present new lithium and v \sin i data for F stars in clusters with ages between the Pleiades and Hyades, and find a strong correlation between the age of the cluster and a) the slope of the trend in this plane, and b) the maximum observed v \sin i for each cluster. We discuss the implications for the mechanisms responsible for the formation of the ``Li Gap''. We gratefully acknowledge support from the National Science Foundation under grant AST 02-06202.
The author(s) of this abstract have provided an email address for comments about the abstract: aaron@astro.indiana.edu
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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.