High-Dispersion Spectra Collection of Nearby F--K Stars at Okayama Astrophysical Observatory: A Basis for Spectroscopic Abundance Standards

Astronomy and Astrophysics – Astronomy

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Astronomical Data Bases: Miscellaneous, Stars: Abundances, Stars: Fundamental Parameters, Stars: Late-Type, Stars: Spectra

Scientific paper

Towards constructing a system of high-dispersion spectroscopic standard stars with well-established abundances, so that adequate reference stars of similar properties may be found for precise differential abundance studies of any near-solar type stars, we have collected high-resolution (R ˜ 70000) echelle spectra for 160 F-K dwarfs and subgiants of the solar neighborhood in three wavelength regions (5000-6200Å, 5800-7000Å, and 7600-8800Å) at Okayama Astrophysical Observatory. This spectra database is open to the public.

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