000002124 001__ 2124
000002124 005__ 20160706150344.0
000002124 0247_ $$2DOI$$a10.1051/0004-6361/201424111
000002124 037__ $$aASTROimport-281
000002124 100__ $$aGrevesse, N.
000002124 245__ $$aThe elemental composition of the Sun. III. The heavy elements Cu to Th
000002124 260__ $$c2015
000002124 520__ $$aWe re-evaluate the abundances of the elements in the Sun from copper (Z = 29) to thorium (Z = 90). Our results are mostly based on neutral and singly-ionised lines in the solar spectrum. We use the latest 3D hydrodynamic solar model atmosphere, and in a few cases also correct for departures from local thermodynamic equilibrium (LTE) using non-LTE (NLTE) calculations performed in 1D. In order to minimise statistical and systematic uncertainties, we make stringent line selections, employ the highest-quality observational data and carefully assess oscillator strengths, hyperfine constants and isotopic separations available in the literature, for every line included in our analysis. Our results are typically in good agreement with the abundances in the most pristine meteorites, but there are some interesting exceptions. This analysis constitutes both a full exposition and a slight update of the relevant parts of the preliminary results we presented in Asplund et al. (2009, ARA, 47, 481), including full line lists and details of all input data that we have employed. Tables 1-3 are available in electronic form at http://www.aanda.org
000002124 700__ $$aScott, P.
000002124 700__ $$aAsplund, M.
000002124 700__ $$aSauval, A. J.
000002124 773__ $$cA27$$pAstronomy and Astrophysics$$v573$$y2015
000002124 85642 $$ahttp://esoads.eso.org/abs/2015A%26A...573A..27G
000002124 905__ $$apublished in
000002124 980__ $$aREFERD