Barker, F C2015-12-132015-12-130375-9474http://hdl.handle.net/1885/94371Data for the 9Be(p, γ)10B reaction with proton energies up to 1800 keV are fitted using R-matrix formulae that include channel contributions where appropriate. The data include values of the astrophysical S factor, the branching ratios for γ-transitions200210.1016/S0375-9474(01)01262-32015-12-12