A redetermination of the solar abundance of molybdenum

Details A redetermination of the solar abundance of molybdenum A redetermination of the solar abundance of molybdenum

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...275..889b&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 275, Dec. 15, 1983, p. 889-891.

Astronomy and Astrophysics

Astrophysics

20

Abundance, Chemical Composition, Molybdenum, Sun, Line Spectra, Solar Spectra, Transition Probabilities

Scientific paper

New accurate transition probabilities are used together with
high-quality solar spectra to derive an improved solar abundance of
molybdenum, AMO = 1.92±0.05.

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