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Autor:
E. Nácher, S. Parra, J.A. Briz, P. Aguilera, J. Agramunt, A. Algora, T. Berry, M.J.G. Borge, M. Carmona, L.M. Fraile, E. Ganioglu, W. Gelletly, V. Guadilla, A. Illana, R. Lică, I. Marroquín, F. Molina, A.I. Morales, N. Orce, S.E.J. Orrigo, A. Perea, J. Romero, B. Rubio, C. Sotty, J.L. Taín, O. Tengblad, A. Tolosa
Publikováno v:
EPJ Web of Conferences. 279:12004
Nucleosynthesis in Type I X-ray bursts (XRB) proceeds eventually through the rp-process near the proton drip-line. Several N=Z nuclei act as waiting points in the reaction network chain. Astrophysical calculations of XRB light curves depend upon the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7f9fd051a9c41ac5d1b2200273c62d2f
https://doi.org/10.1051/epjconf/202327912004
https://doi.org/10.1051/epjconf/202327912004
