Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...274..391s&link_type=abstract
Astronomy and Astrophysics, Vol. 274, NO. 2/JUL(II), P. 391, 1993
Astronomy and Astrophysics
Astrophysics
60
Stars: Abundances, Stars: Chemically Peculiar, Techniques: Photometric, Techniques: Spectroscopic
Scientific paper
Medium-resolution spectra have been used to determine values of mean metal abundance ([M/H]) for 28 A-type stars, including several metal-rich metallic-lined (Am) stars, by spectrum synthesis techniques. A new calibration of the Strömgren metallicity index (δm0) with [M/H], valid for A3 - F0 stars (2.72 < β < 2.88), is obtained: [M/H] = -1O.56δm0 +0.081.
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