Oxygen Abundances of Solar-Type Dwarfs in Open Clusters: M34 and the Pleiades

Details Oxygen Abundances of Solar-Type Dwarfs in Open Clusters: M34 and the Pleiades Oxygen Abundances of Solar-Type Dwarfs in Open Clusters: M34 and the Pleiades

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...202.2707s&link_type=abstract

American Astronomical Society Meeting 202, #27.07; Bulletin of the American Astronomical Society, Vol. 35, p.734

Astronomy and Astrophysics

Astronomy

Scientific paper

We present 7774 ; Å O 1 triplet oxygen abundances derived from Keck/HIRES and HET/HRS spectra of numerous solar-type dwarfs in open clusters M34 and the Pleiades. This represents the first analysis of O in a significant number of cool open cluster dwarfs. We discuss the results and any correlations of the O abundances, as well as implications for chromospherically induced NLTE effects. This work has been generously supported by NSF grant AST00-86576 to JRK.

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