HST/STIS abundances in the uranium rich metal poor star CS 31082-001: Constraints on the r-Process
[发布日期] [发布机构] IAG, Universidade de São Paulo, Cidade Universitária, Rua do Matão 1226, São Paulo; 05508-900, Brazil^1;GEPI, Observatoire de Paris, CNRS, UMR 8111, Meudon Cedex; 92195, France^2;Zentrum für Astronomie, Universität Heidelberg, Landessternwarte, Königstuhl 12, Heidelberg; 69117, Germany^3;Laboratoire Lagrange, UMR 7293, Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, Nice; 06300, France^4;National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo; 181-8588, Japan^5;European Southern Observatory, Karl Schwarzschild Strasse 2, Garching bei München; 85748, Germany^6;LUPM, CNRS, UMR 5299, Université de Montpellier II, Montpellier Cedex 05; 34095, France^7;GEPI, Observatoire de Paris, CNRS, UMR 8111, 61 Av. de l'Observatoire, Paris; 75014, France^8;Niels Bohr Institute, Juliane Maries Vej 30, Copenhagen; 2100, Denmark; (10) Nordic Optical Telescope, Apartado 474, Santa Cruz de La Palma; 38700, Spain; (11) University of Texas at Austin, Department of Astronomy, Austin; TX; 78712, United States; (12) National Optical Astronomy Observatory, Tucson; MI; 85719, United States; (13) Michigan State University, Department of Physics and Astronomy, JINA, Joinst Institute for Nuclear Physics, East Lansing; MI; 48824, United States; (14) INAF, Osservatorio Astronomico di Trieste, via Tiepolo 11, Trieste; 34143, Italy^9
[效力级别] 天文学 [学科分类] 天文学(综合)
[关键词] Element abundances;Heavy elements;Metal-poor star;Near uv;Neutron exposure;Nuclear data;R-process [时效性]