Uncertainties in the solar system r-abundance distribution

Details Uncertainties in the solar system r-abundance distribution Uncertainties in the solar system r-abundance distribution

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26a...342..881g&link_type=abstract

Astronomy and Astrophysics, v.342, p.881-891 (1999)

Astronomy and Astrophysics

Astrophysics

24

Nuclear Reactions, Nucleosynthesis, Abundances, Sun: Abundances, Solar System: General, Stars: Abundances

Scientific paper

The solar system r-abundance distribution is commonly derived from the observed solar values by subtracting the possible nucleosynthetic contribution of the s-process. The new parametric model of the s-process called the canonical multi-event model is used to derive the s-component of the solar abundance distribution and to study the impact of nuclear and observational uncertainties on the solar r-abundance distribution. Tables 1 and 2 are only available in electronic form at the CDS (Strasbourg) via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/Abstract.html

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