Click here to close this panel.
S. J. Adelman1 and M. A. Nasson1
© 1980. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A.
,
,
Citation S. J. Adelman and M. A. Nasson 1980 PASP 92 346
DOI 10.1086/130675
65 Total downloads
Abundance analyses for three moderately sharp-lined stars with spectral types near AO Theta Aql, Nu Cap, and Sigma Aqr have been performed via model atmospheres techniques. The derived abundances of the first two stars are quite similar to those of the sun and other normal main-sequence stars. Those of Sigma Aqr suggest that this star is a hot metallic-line star.
