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

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

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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