Abundances of singly-ionized elements of the iron group in the sun

Astronomy and Astrophysics – Astronomy

Scientific paper

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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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