Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184..683b&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 184, Sept. 1978, p. 683-694. Research supported by the Fonds de la Rech
Astronomy and Astrophysics
Astronomy
19
Abundance, Iron, Solar Atmosphere, Solar Spectra, Atmospheric Composition, Iterative Solution, Line Spectra, Oscillators, Photosphere, Spectral Line Width, Spectrum Analysis, Stellar Models, Tables (Data)
Scientific paper
Abundances of the iron-group elements are derived from ionic lines present in the solar photospheric spectrum. Within the precision permitted by our present knowledge of f values, atmospheric models, and damping theory, equivalent-width procedure or spectrum-synthesis analysis lead to abundances in harmony with those found from neutral species and with the results available from the study of carbonaceous chondrites.
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