NSR Query Results
Output year order : Descending NSR database version of May 6, 2024. Search: Author = C.Sneden Found 12 matches. 2021CO05 Rev.Mod.Phys. 93, 015002 (2021) J.J.Cowan, C.Sneden, J.E.Lawler, A.Aprahamian, M.Wiescher, K.Langanke, G.Martinez-Pinedo, F.-K.Thielemann Origin of the heaviest elements: The rapid neutron-capture process
doi: 10.1103/RevModPhys.93.015002
2021DE27 Astrophys.J.Suppl.Ser. 255, 27 (2021) E.A.Den Hartog, J.E.Lawler, C.Sneden, J.J.Cowan, I.U.Roederer, J.Sobeck Atomic Transition Probabilities of Neutral Calcium ATOMIC PHYSICS Ca; analyzed available theoretical and experimental data; deduced new radiative lifetimes, new emission branching fractions.
doi: 10.3847/1538-4365/ac04b1
2017LA13 Can.J.Phys. 95, 783 (2017) J.E.Lawler, C.Sneden, J.J.Cowan, E.A.Den Hartog, M.P.Wood Laboratory transition probabilities for studies of nucleosynthesis of Fe-group elements ATOMIC PHYSICS Sc, Ti, V, Cr, Mn, Fe, Co, Ni; compiled measurements of γ-rays, X-rays and visible light; deduced elemental abundances.
doi: 10.1139/cjp-2016-0689
2014RO06 Astrophys.J. 784, 158 (2014) I.U.Roederer, G.W.Preston, I.B.Thompson, S.A.Shectman, C.Sneden Neutron-capture Nucleosynthesis in the First Stars
doi: 10.1088/0004-637X/784/2/158
2013LA12 Astrophys.J.Suppl.Ser. 205, 11 (2013) J.E.Lawler, A.Guzman, M.P.Wood, C.Sneden, J.J.Cowan Improved Log(gf) Values for Lines of Ti I and Abundance Determinations in the Photospheres of the Sun and Metal-Poor Star HD 84937 (Accurate Transition Probabilities for Ti I) ATOMIC PHYSICS Ti; measured Fourier transform spectra, laser-induced fluorescence; deduced atomic transition probabilities, log gt. Comparison with available data.
doi: 10.1088/0067-0049/205/2/11
2009RO11 Astrophys.J. 698, 1963 (2009) I.U.Roederer, K.-L.Kratz, A.Frebel, N.Christlieb, B.Pfeiffer, J.J.Cowan, C.Sneden The End of Nucleosynthesis: Production of Lead and Thorium in the Early Galaxy
doi: 10.1088/0004-637X/698/2/1963
2008SN01 Ann.Rev.Astron.Astrophys. 46, 241 (2008) C.Sneden, J.J.Cowan, R.Gallino Neutron-Capture Elements in the Early Galaxy NUCLEAR REACTIONS 69,71Ga, 70,72,73,74,76Ge, 75As, 76,77,78,80,82Se, 79,81Br, 80,82,83,84,86Kr, 85,87Rb, 86,87,88Sr, 89Y, 90,91,92,94,96Zr, 93Nb, 95,96,97,98,100Mo, 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, 128,129,130,131,132,134Xe, 133Cs, 134,135,136,137,138Ba, 139La, 140,142Ce, 141Pr, 142,143,144,145,146,148,150Nd, 147,148,149,150,152,154Sm, 151,153Eu, 152,154,155,156,157,158,160Gd, 159Tb, 160,161,162,163,164Dy, 165Ho, 164,166,167,168,170Er, 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, 232Th, 235,238U(n, γ), E ∼ 30 keV; analyzed available data; deduced s- and r-process abundances.
doi: 10.1146/annurev.astro.46.060407.145207
2007KR20 Astrophys.J. 662, 39 (2007) K.-L.Kratz, K.Farouqi, B.Pfeiffer, J.W.Truran, C.Sneden, J.J.Cowan Explorations of the r-Processes: Comparisons between Calculations and Observations of Low-Metallicity Stars NUCLEAR REACTIONS 138Ba(n, γ), E ∼ 30 keV; analyzed available data; calculated r-process abundances in low-metallicity stars.
doi: 10.1086/517495
2006CO25 Nature(London) 440, 1151 (2006) Heavy element synthesis in the oldest stars and the early Universe
doi: 10.1038/nature04807
2004TR05 Astrophys.J. 601, 864 (2004) C.Travaglio, R.Gallino, E.Arnone, J.Cowan, F.Jordan, C.Sneden Galactic evolution of Sr, Y, and Zr: A multiplicity of nucleosynthetic processes
doi: 10.1086/380507
2003SN02 Nucl.Phys. A718, 29c (2003) C.Sneden, J.J.Cowan, J.E.Lawler Observations of Neutron-Capture Elements in the Early Galaxy
doi: 10.1016/S0375-9474(03)00676-6
1997CO17 Nucl.Phys. A621, 41c (1997) J.J.Cowan, C.Sneden, J.W.Truran, D.L.Burris, A.McWilliam, G.W.Preston R- and S-Process Signatures in Metal-Poor Halo Stars
doi: 10.1016/S0375-9474(97)00209-1
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