F-values and abundances of the elements in the sun and stars

Details F-values and abundances of the elements in the sun and stars F-values and abundances of the elements in the sun and stars

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977phys...16...39b&link_type=abstract

Physica Scripta, vol. 16, July-Aug. 1977, p. 39-47. Research supported by the Fonds National de la Recherche Scientifique.

Astronomy and Astrophysics

Astrophysics

31

Abundance, Astronomical Spectroscopy, Chemical Elements, Solar Spectra, Stellar Atmospheres, Stellar Spectra, Atomic Spectra, Chemical Composition, Molecular Spectra, Photosphere, Stellar Models, Thermodynamic Equilibrium

Scientific paper

The article reviews the atomic and molecular f-values currently needed to determine solar abundances. The abundances of chemical elements in stellar objects are discussed along with a photospheric model, local thermodynamic equilibrium, line opacity, and spectrum synthesis. The oscillator strengths required for small astrophysical models are described, and various problems encountered in stellar spectroscopy are outlined.

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