Spectroscopic Abundances of Solar Type Dwarfs in the Open Cluster M34

Details Spectroscopic Abundances of Solar Type Dwarfs in the Open Cluster M34 Spectroscopic Abundances of Solar Type Dwarfs in the Open Cluster M34

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...199.5709s&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #57.09; Bulletin of the American Astronomical Society, Vol. 33, p.1388

Astronomy and Astrophysics

Astronomy

Scientific paper

Abundances of numerous elements are derived for several solar-type dwarfs in the young open cluster M34 from high-resolution (R ~45,000) Keck/HIRES spectra. Results are presented and discussed to address their implications for intra-cluster abundance scatter, Galactic chemical evolution, and stellar Li depletion. This work was supported by NSF grant AST-0086576 to JRK.

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