Abundances of singly-ionized elements of the iron group in the Sun.
Abstract
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.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- September 1978
- DOI:
- 10.1093/mnras/184.4.683
- Bibcode:
- 1978MNRAS.184..683B
- Keywords:
-
- Abundance;
- Iron;
- Solar Atmosphere;
- Solar Spectra;
- Atmospheric Composition;
- Iterative Solution;
- Line Spectra;
- Oscillators;
- Photosphere;
- Spectral Line Width;
- Spectrum Analysis;
- Stellar Models;
- Tables (Data);
- Solar Physics;
- Element Abundances:Solar Photosphere