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Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions. (arXiv:1705.03642v1 [astro-ph.SR])
- Volume 12, Issue 19 - article #2
- T. Mishenina (1), M. Pignatari (2,3,6), B.Cot'e (3,4,5,6), F.-K. Thielemann (7), C. Soubiran (8), N. Basak (1), T. Gorbaneva (1), S.A. Korotin (1,9), V.V. Kovtyukh (1), B. Wehmeyer (7), S. Bisterzo (3,10,11), C. Travaglio (3,10,11), B.K. Gibson (2,6), C. Jordan (2,6), A. Paul (4), C. Ritter (3,6), F. Herwig (3,6) ((1) Astronomical Observatory, Odessa National University,, Isaac Newton Institute of Chile, Odessa branch, Odessa, Ukraine, (2) E.A. Milne Centre for Astrophysics, University of Hull, (3) The NuGrid Collaboration, (4) Department of Physics, Astronomy, University of Victoria, (5) National Superconducting Cyclotron Laboratory, Michigan State University, (6) Joint Institute for Nuclear Astrophysics Center for the Evolution of the Elements, (7) Department of Physics, University of Basel, (8) Laboratoire d'Astrophysique de Bordeaux, Univ. Bordeaux - CNRS, B18N, allée Geoffroy Saint-Hilaire, (9) Crimean Astrophysical Observatory, (10) INAF, Astrophysical Observatory Turin, Strada Osservatorio 20, (11) B2FH Association)
- http://arxiv.org/abs/1705.03642