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Almudena Arcones

Almudena Arcones Segovia (born 1979) is a Spanish-German nuclear astrophysicist whose research topics have included the creation and decay of heavy elements through the ''r''-process, and neutrino-driven outflows, in energetic stellar events including supernovae and neutron star mergers. She is a professor of theoretical astrophysics at Technische Universität Darmstadt in Germany, and a researcher in the GSI Helmholtz Centre for Heavy Ion Research in Darmstadt. Provided by Wikipedia
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    Chemical evolution of R-process elements in stars (CERES) - I. stellar parameters and chemical abundances from Na to Zr by Lombardo, Linda (Author) , Bonifacio, Piercarlo (Author) , François, Patrick (Author) , Hansen, Camilla J. (Author) , Caffau, Elisabetta (Author) , Hanke, Michael (Author) , Ása Skúladóttir (Author) , Arcones, Almudena (Author) , Eichler, Marius (Author) , Reichert, Moritz (Author) , Psaltis, Athanasios (Author) , Koch-Hansen, Andreas (Author) , Sbordone, Luca (Author) ,


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