NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = J.J.Cowan 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
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
2012SA07 Rep.Prog.Phys. 75, 036901 (2012) D.W.Savin, N.S.Brickhouse, J.J.Cowan, R.P.Drake, S.R.Federman, G.J.Ferland, A.Frank, M.S.Gudipati, W.C.Haxton, E.Herbst, S.Profumo, F.Salama, L.M.Ziurys, E.G.Zweibel The impact of recent advances in laboratory astrophysics on our understanding of the cosmos
doi: 10.1088/0034-4885/75/3/036901
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
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
2001TR15 Nucl.Phys. A688, 330c (2001) J.W.Truran, J.J.Cowan, B.D.Fields Halo Star Abundances and r-Process Synthesis
doi: 10.1016/S0375-9474(01)00722-9
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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