NSR Query Results
Output year order : Descending NSR database version of May 8, 2024. Search: Author = V.Antonuccio-Delogu Found 1 matches. 2021BU01 Astrophys.J. 908, 55 (2021) M.Busso, D.Vescovi, S.Palmerini, S.Cristallo, V.Antonuccio-Delogu s-processing in AGB Stars Revisited. III. Neutron Captures from MHD Mixing at Different Metallicities and Observational Constraints NUCLEAR REACTIONS 58Fe, 64Ni, 63,65Cu, 64,66,67,68,70Zn, 69,71Ga, 70,72,73,74,76Ge, 75As, 76,77,78,82Se, 79,81Br, 80,82,83,84,86Kr, 85,87Rb, 86,87,88Sr, 89Y, 90,91,92,94,96Zr, 93Nb, 96,97,98Mo, 99,100,101,102,104Ru, 103Rh, 104,105,106,108,110Pd, 107,109Ag, 110,111,112,113,114,116Cd, 115In, 116,117,118,119,120,122,124Sn, 121,123Sb, 122,123,124,125,126,128,130Te, 127I, 128,129,130,131,132,134,136Xe, 133Cs, 134,135,136,137,138Ba, 139La, 140,142Ce, 141Pr, 142,143,144,145,146,148,150Nd, 147,148,149,150,152Sm, 151,153Eu, 152,154,155,156,157,158,160Gd, 159Tb, 160,161,162,163,164Dy, 165Ho, 166,167,168,170Er, 169Tm, 170,171,172,173,174,176Yb, 175,176Lu, 176,177,178,179,180Hf, 181Ta, 182,183,184,186W, 185,187Re, 186,187,188,189,190,192Os, 191,193Ir, 192,194,195,196,198Pt, 197Au, 198,199,200,201,202,204Hg, 203,205Tl, 204,206,207,208Pb, 209Bi(n, γ), E ∼ 30 keV; calculated s-process main component solar system abundances.
doi: 10.3847/1538-4357/abca8e
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