Marganiec, J.Wamers, F.Aksouh, F.Aksyutina, Y.Álvarez Pol, HéctorAumann, T.Beceiro Novo, SaúlBertulani, C. A.Boretzky, K.Borge, M. J. G.Chartier, M.Chatillon, A.Chulkov, L. V.Cortina Gil, María DoloresEmling, H.Ershova, O.Fraile, L. M.Fynbo, H. O. U.Galaviz, D.Geissel, H.Heil, M.Hoffmann, D. H. H.Hoffmann, J.Johansson, H. T.Jonson, B.Karagiannis, C.Kiselev, O. A.Kratz, J. V.Kulessa, R.Kurz, N.Langer, C.Lantz, M.Le Bleis, T.Lemmon, R.Litvinov, Yu. A.Mahata, K.Müntz, C.Nilsson, T.Nociforo, C.Nyman, G.Ott, W.Panin, V.Paschalis, S.Perea, A.Plag, R.Reifarth, R.Richter, A.Rodríguez Tajes, CarmeRossi, D.Riisager, K.Savran, D.Schrieder, G.Simon, H.Stroth, J.Sümmerer, K.Tengblad, O.Typel, S.Weick, H.Wiescher, M.Wimmer, C.2020-06-052020-06-052016Marganiec, J., Wamers, F., Aksouh, F., Aksyutina, Y., Álvarez-Pol, H., Aumann, T., ... & Chartier, M. (2016). Coulomb and nuclear excitations of narrow resonances in 17Ne. Physics Letters B, 759, 200-2050370-2693http://hdl.handle.net/10347/22788New experimental data for dissociation of relativistic 17Ne projectiles incident on targets of lead, carbon, and polyethylene targets at GSI are presented. Special attention is paid to the excitation and decay of narrow resonant states in 17Ne. Distributions of internal energy in the 15O +p +pthree-body system have been determined together with angular and partial-energy correlations between the decay products in different energy regions. The analysis was done using existing experimental data on 17Ne and its mirror nucleus 17N. The isobaric multiplet mass equation is used for assignment of observed resonances and their spins and parities. A combination of data from the heavy and light targets yielded cross sections and transition probabilities for the Coulomb excitations of the narrow resonant states. The resulting transition probabilities provide information relevant for a better understanding of the 17Ne structure.eng© 2016 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP3http://creativecommons.org/licenses/by/4.0/journal article10.1016/j.physletb.2016.05.0731873-2445open access