Stellar and Solar Abundances

Computer Science

Scientific paper

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Scientific paper

Recent spectroscopic results on stellar and solar abundances are reviewed with special reference to (a) Standard abundance distribution (Sun, hot stars, diffuse nebulae); (b) Abundance peculiarities related to stellar evolution (red giants showing results of H-burning and s-process, peculiar and metallic-lined stars); and (c) Population effects that may be related to the evolution of the Galaxy (correlation between stellar age and metal abundance, differences in details of heavyelement mixture in atmospheric composition of normal stars that have not reached an advanced evolutionary stage).

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