Uncertainties in the solar system r-abundance distribution

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