High-resolution spectral analysis of the mildly metal-poor stars I. Spectral data and equivalent widths

Details High-resolution spectral analysis of the mildly metal-poor stars I. Spectral data and equivalent widths High-resolution spectral analysis of the mildly metal-poor stars I. Spectral data and equivalent widths

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002acasn..43..113z&link_type=abstract

Acta Astronomica Sinica, vol.43, no.2, p.113-120

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1

Stars: Abundances, Stars: Evolution, Line: Profiles

Scientific paper

The high resolution, high signal to noise ratio spectra of a sample of mildly metal-poor stars were obtained with the Coude Echelle Spectrograph attached to the 2.16m telescope at Beijing Astronomical Observatory (Xinglong, China). The spectra are reduced with the MIDAS package and the equivalent widths of seven stars were measured. The error of the equivalent widths is estimated by comparing them with the other independent measurements made by the other authors. The standard deviations are presented in the end.

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