J/A+A/487/767ivo://CDS.VizieR/J/A+A/487/767doi:10.26093/cds/vizier.34870767CDSGoriely S.Hilaire S.Koning A.J.2008-11-16T08:56:38Z2008-11-16T09:50:57ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fratomic-physicsNuclear reaction rates of astrophysical applications are traditionally determined on the basis of Hauser-Feshbach reaction codes. These codes adopt a number of approximations that have never been tested, such as a simplified width fluctuation correction, the neglect of delayed or multiple-particle emission during the electromagnetic decay cascade, or the absence of the pre-equilibrium contribution at increasing incident energies. The reaction code TALYS has been recently updated to estimate the Maxwellian-averaged reaction rates that are of astrophysical relevance. These new developments enable the reaction rates to be calculated with increased accuracy and reliability and the approximations of previous codes to be investigated.2008A&A...487..767Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/487/767CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/287/927 : Abundances for lines of n-capture in 19 stars (Gratton+ 1994)J/AZh/81/209 : Neutron capture elements in stars: neodymium (Mashonkina+ 2004)J/AZh/84/429 : Abundances in atmospheres of cool giants (Mishenina+, 2007)J/AZh/84/997 : Neutron capture elements in halo+disk stars (Mashonkina+, 2007)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/487/767https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/487/767http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/487/767https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/487/767https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/487/767http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/487/767GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/487/767/ratesMaxwellian-averaged nuclear reaction ratesFileOriginal file name (1)meta.id;meta.filecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAMass number of the target nucleusphys.atmol.numberintprimaryZSymbol of the target nucleusphys.atmol.elementcharprimaryp[anp] projectile (2)phys.atmol.elementcharprimarye1[agnp] ejectile in first reaction (2)phys.atmol.elementcharprimaryA1Mass number of the residual in first reactionphys.atmol.numberintZ1Symbol of the residual nucleusphys.atmol.elementchare2[agnp] ejectile in second reaction (2)phys.atmol.elementcharA2Mass number of the residual nucleusphys.atmol.numberintZ2Symbol of the residual nucleusphys.atmol.elementchare3[agnp] ejectile in third reaction (2)phys.atmol.elementcharA3Mass number of the residual nucleusphys.atmol.numberintZ3Symbol of the residual nucleusphys.atmol.elementcharT9Temperature of the reaction1e+09Kphys.temperature;meta.mainfloatprimaryRate1Rate of reaction 1: A.Z (p,e1) A1.Z1cm**3.mol**-1.s**-1meta.notedoubleRate2Rate of reaction 2: A.Z (p,e2) A2.Z2cm**3.mol**-1.s**-1meta.notedoubleRate3Rate of reaction 3: A.Z (p,e3) A3.Z3cm**3.mol**-1.s**-1meta.notedouble