Enrichment of the Galactic Disc with Neutron-Capture Elements: Mo and Ru
This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record is available online at: https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stz2202/5548790 Enrichment of the Galactic disc with neutron-capture Downloaded from https://academic.oup.com/mnras/advance-article-abstract/doi/10.1093/mnras/stz2202/5548790 by University of Hull user on 14 August 2019 elements: Mo and Ru T. Mishenina1 ⋆, M. Pignatari2,3,6 † *, T. Gorbaneva1, C. Travaglio4,5 † , B. Cˆot´e3,6 † , F.-K. Thielemann7,8, C. Soubiran9 1Astronomical Observatory, Odessa National University, Shevchenko Park, 65014, Odessa, Ukraine 2 E.A. Milne Centre for Astrophysics, Dept of Physics & Mathematics, University of Hull, HU6 7RX, United Kingdom 3 Konkoly Observatory, Hungarian Academy of Sciences, Konkoly Thege Miklos ut 15-17, H-1121 Budapest, Hungary 4 INFN, University of Turin, Via Pietro Giuria 1, 10025 Turin, Italy 5 B2FH Association, Turin, Italy 6 Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements, USA 7 Department of Physics, University of Basel, Klingelbergstrabe 82, 4056 Basel, Switzerland 8 GSI Helmholtzzentrum fr Schwerionenforschung, Planckstrasse 1, D-64291 Darmstadt, Germany 9 Laboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux - CNRS, B18N, all´ee Geoffroy Saint-Hilaire, 33615 Pessac, France Accepted 2015 xxx. Received 2015 xxx; in original form 2015 xxx ABSTRACT We present new observational data for the heavy elements molybdenum (Mo, Z = 42) and ruthenium (Ru, Z = 44) in F-, G-, and K-stars belonging to different substructures of the Milky Way.
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