IOP Publishing, Journal of Physics: Conference Series, (202), p. 012021, 2010
DOI: 10.1088/1742-6596/202/1/012021
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The indirect measurement of 17O(p,α)14N cross section was performed by means of the Trojan Horse Method. This approach allowed to investigate the ultra-low energy range (Ec.m. = 0-300 keV) relevant for several astrophysics environments, where two resonant levels of 18F at ERc.m. = 65 keV and ERc.m. = 183 keV play a significant role in the reaction rate determination.