Physics
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005noao.prop..268s&link_type=abstract
NOAO Proposal ID #2005B-0268
Physics
Scientific paper
The vexing problem of the enormous Li dispersion observed in the Pleiades G & K dwarfs continues to confound us more than 20 years after its initial discovery. It remains unclear if the dispersion is a result of real Li abundance differences, possibly due to rotational effects, or if it is illusory, perhaps related to chromospheric activity and/or photospheric spots. It is critically important to distinguish between these two scenarios, or the uncertainty will seriously restrict the irreplaceable use of Li as a probe of stellar interiors in young G & K dwarfs. We propose a combined long- and short-term program that will definitively determine whether or not activity and/or spots affect Li line strengths, and if they do, to quantify the degree of the effect. The long-term project will use WIYN 3.5m/Hydra to monitor efficiently and simultaneously the (lambda) 6707 Li I feature, the similarly formed (lambda) 7699 K I feature, and activity indicators in 43 G & K Pleiades dwarfs over a five year period, looking for possible correlated variations. The short-term project will utilize both WIYN 3.5m/Hydra and WIYN 0.9m/MOSAIC to look for line variations and correlated photometric variations, which are good indicators of spots, over a short period of four nights.
Barnes Sydney A.
Deliyannis Constantine P.
Kafka Styliani
King Jeremy R.
Schuler Simon C.
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