Published in
Kluwer, Symposium- International Astronomical Union, (213), p. 55-58, 2004
DOI: 10.1017/s0074180900192964
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Refining the Search for ^6Li in Stars with Planets
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Abstract
The primary conflict between studies attempting to measure 6Li in stars harboring planets, a potential indicator of planet formation, is the incompleteness and inaccuracy of current line lists for the lithium region. We are attempting to resolve these issues using very high-resolution (R ∼ 120,000) and very high quality (S/N between 250 and 1000) spectra of stars with a range of abundances.