Cortés Giraldo, Miguel AntonioPraena Rodríguez, JavierQuesada Molina, José ManuelSabaté Gilarte, MartaMingrone, FMassimi, C.Vannini, Gianni2016-11-302016-11-302014Cortés Giraldo, M.A., Praena Rodríguez, J., Quesada Molina, J.M., Sabaté Gilarte, M., Mingrone, F., Massimi, C. y Vannini, G. (2014). The nucleosynthesis of heavy elements in stars: the key isotope 25Mg. EPJ Web of Conferences, 66, 07016-1-07016-4.2100-014Xhttp://hdl.handle.net/11441/49382INPC 2013 – International Nuclear Physics ConferenceWe have measured the radiative neutron-capture cross section and the total neutron-induced cross section of one of the most important isotopes for the s process, the 25Mg. The measurements have been carried out at the neutron time-of-flight facilities n_TOF at CERN (Switzerland) and GELINA installed at the EC-JRC-IRMM (Belgium). The cross sections as a function of neutron energy have been measured up to approximately 300 keV, covering the energy region of interest to the s process. The data analysis is ongoing and preliminary results show the potential relevance for the s processapplication/pdfengAttribution-NonCommercial-NoDerivatives 4.0 Internacionalhttp://creativecommons.org/licenses/by-nc-nd/4.0/The nucleosynthesis of heavy elements in stars: the key isotope 25Mginfo:eu-repo/semantics/articleinfo:eu-repo/semantics/openAccesshttps://doi.org/10.1051/epjconf/20146607016