Abundance analyses of Theta Aquilae /B9.5 III/, Nu Capricorni /B9.5 V/, and Sigma Aquarii /AO IVs/

Details Abundance analyses of Theta Aquilae /B9.5 III/, Nu Capricorni /B9.5 V/, and Sigma Aquarii /AO IVs/ Abundance analyses of Theta Aquilae /B9.5 III/, Nu Capricorni /B9.5 V/, and Sigma Aquarii /AO IVs/

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pasp...92..346a&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 92, June 1980, p. 346-356.

Other

10

A Stars, Abundance, B Stars, Line Spectra, Stellar Atmospheres, Stellar Spectra, Chemical Composition, Hot Stars, Main Sequence Stars, Metallic Stars, Solar Spectra, Spectroscopic Analysis, Stellar Temperature, Tables (Data)

Scientific paper

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.

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