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NSR database version of April 11, 2024.

Search: Author = R.Gallino

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2023GA10      Eur.Phys.J. A 59, 66 (2023)

R.Gallino

Franz and his friends: 35-years of s-process studies by the Karlsruhe-Torino collaboration

doi: 10.1140/epja/s10050-023-00934-8
Citations: PlumX Metrics


2023PI08      Eur.Phys.J. A 59, 302 (2023)

M.Pignatari, R.Gallino, R.Reifarth

The s process in massive stars, a benchmark for neutron capture reaction rates

doi: 10.1140/epja/s10050-023-01206-1
Citations: PlumX Metrics


2022LI64      Eur.Phys.J. A 58, 216 (2022)

N.Liu, T.Stephan, S.Cristallo, D.Vescovi, R.Gallino, L.R.Nittler, C.M.O.D.Alexander, A.M.Davis

Presolar silicon carbide grains of types Y and Z: their strontium and barium isotopic compositions and stellar origins

doi: 10.1140/epja/s10050-022-00838-z
Citations: PlumX Metrics


2014BI20      Astrophys.J. 787, 1 (2014)

S.Bisterzo, C.Travaglio, R.Gallino, M.Wiescher, F.Kappeler

Galactic chemical evolution and solar s-process abundances: dependence on the 13C-pocket structure

NUCLEAR REACTIONS 80,82,83,84,86Kr, Kr, 85,87Rb, Rb, 86,87,88Sr, Sr, 89Y, Y, 90,91,92,94,96Zr, Zr, 93Nb, Nb, 94,95,96,97,98,100Mo, Mo, 99,100,101,102,104Ru, Ru, 103Rh, Rh, 104,105,106,108,110Pd, Pd, 107,109Ag, Ag, 108,110,111,112,113,114,116Cd, Cd, 113,115In, In, 114,115,116,117,118,119,120,122,124Sn, Sn, 121,123Sb, Sb, 122,123,124,125,126,128Te, Te, 127I, I, 128,129,130,131,132,134Xe, Xe, 133Cs, Cs, 134,135,136,137,138Ba, Ba, 139La, La, 140,142Ce, Ce, 141Pr, Pr, 142,143,144,145,146,148Nd, Nd, 147,148,149,150,152,154Sm, Sm, 151,153Eu, Eu, 152,154,155,156,157,158,160Gd, Gd, 159Tb, Tb, 160,161,162,163,164Dy, Dy, 165Ho, Ho, 164,166,167,168,170Er, Er, 169Tm, Tm, 170,171,172,173,174,176Yb, Yb, 175,176Lu, Lu, 176,177,178,179,180Hf, Hf, 180,181Ta, Ta, 180,182,183,184,186W, W, 185,187Re, Re, 186,187,188,189,190,192Os, Os, 191,193Ir, Ir, 192,194,195,196,198Pt, Pt, 197Au, Au, 198,199,200,201,202,204Hg, Hg, 203,205Tl, Tl, 204,206,207,208Pb, Pb, 209Bi, Bi(n, γ), E ∼ 30 keV; analyzed available data; deduced s-process abundances.

doi: 10.1088/0004-637x/787/1/10
Citations: PlumX Metrics


2014HE25      Phys.Rev. C 90, 045804 (2014); Erratum Phys.Rev. C 92, 019902 (2015)

M.Heil, R.Plag, E.Uberseder, R.Gallino, S.Bisterzo, A.Juseviciute, F.Kappeler, C.Lederer, A.Mengoni, M.Pignatari

Stellar neutron capture cross sections of 20, 21, 22Ne

NUCLEAR REACTIONS 20,21,22Ne(n, γ), E=5-800 keV; measured transmission data, σ(E) via prompt γ-ray cascades, and using the TOF technique at the Karlsruhe Van de Graaff accelerator. 21,22,23Ne; deduced energies of neutron resonances, resonance parameters, widths, capture kernels, stellar cross sections (MACS) at kT=30 keV, relative s-abundance distributions. R-matrix analysis using SAMMY code. Comparison with previous experimental results and data in KADONIS database. Discussed 22Ne and 20Ne as significant neutron poisons for the s process in stars.

doi: 10.1103/PhysRevC.90.045804
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23265. Data from this article have been entered in the XUNDL database. For more information, click here.


2011KA13      Rev.Mod.Phys. 83, 157 (2011)

F.Kappeler, R.Gallino, S.Bisterzo, W.Aoki

The s process: Nuclear physics, stellar models, and observations

doi: 10.1103/RevModPhys.83.157
Citations: PlumX Metrics


2011TA17      Phys.Rev. C 84, 015801 (2011)

G.Tagliente, P.M.Milazzo, K.Fujii, U.Abbondanno, G.Aerts, H.Alvarez, F.Alvarez-Velarde, S.Andriamonje, J.Andrzejewski, L.Audouin, G.Badurek, P.Baumann, F.Becvar, F.Belloni, E.Berthoumieux, S.Bisterzo, F.Calvino, M.Calviani, D.Cano-Ott, R.Capote, C.Carrapico, P.Cennini, V.Chepel, E.Chiaveri, N.Colonna, G.Cortes, A.Couture, J.Cox, M.Dahlfors, S.David, I.Dillmann, C.Domingo-Pardo, W.Dridi, I.Duran, C.Eleftheriadis, M.Embid-Segura, A.Ferrari, R.Ferreira-Marques, W.Furman, R.Gallino, I.Goncalves, E.Gonzalez-Romero, F.Gramegna, C.Guerrero, F.Gunsing, B.Haas, R.Haight, M.Heil, A.Herrera-Martinez, E.Jericha, F.Kappeler, Y.Kadi, D.Karadimos, D.Karamanis, M.Kerveno, E.Kossionides, M.Krticka, C.Lamboudis, H.Leeb, A.Lindote, I.Lopes, M.Lozano, S.Lukic, J.Marganiec, S.Marrone, T.Martnez, C.Massimi, P.Mastinu, A.Mengoni, C.Moreau, M.Mosconi, F.Neves, H.Oberhummer, S.O'Brien, J.Pancin, C.Papachristodoulou, C.Papadopoulos, C.Paradela, N.Patronis, A.Pavlik, P.Pavlopoulos, L.Perrot, M.T.Pigni, R.Plag, A.Plompen, A.Plukis, A.Poch, J.Praena, C.Pretel, J.Quesada, T.Rauscher, R.Reifarth, M.Rosetti, C.Rubbia, G.Rudolf, P.Rullhusen, J.Salgado, C.Santos, L.Sarchiapone, I.Savvidis, C.Stephan, J.L.Tain, L.Tassan-Got, L.Tavora, R.Terlizzi, G.Vannini, P.Vaz, A.Ventura, D.Villamarin, M.C.Vincente, V.Vlachoudis, R.Vlastou, F.Voss, S.Walter, M.Wiescher, K.Wisshak

Neutron capture on 94Zr: Resonance parameters and Maxwellian-averaged cross sections

NUCLEAR REACTIONS 94Zr(n, γ), E=0.001-60 keV; measured E(n), I(n), capture yield using CERN n_TOF neutron source; deduced resonance parameters ER, gamma and neutron widths, capture kernels; calculated Maxwellian-averaged capture cross sections. 95Zr; deduced resonances, J, l-values, R-matrix analysis. Comparison with previous studies. Discussed astrophysical implications.

doi: 10.1103/PhysRevC.84.015801
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23330. Data from this article have been entered in the XUNDL database. For more information, click here.


2010CR05      J.Phys.:Conf.Ser. 202, 012033 (2010)

S.Cristallo, L.Piersanti, R.Gallino, O.Straniero, F.Kappeler, I.Dominguez, P.Mohr

The long-standing problem of 176Lu/176Hf branching: A new approach with full stellar evolutionary models

NUCLEAR REACTIONS 175Lu(n, γ), E above 15 keV; calculated long-term time behaviour of 176Lu and 176Hf [product of β-decay of excited 176Lu].

doi: 10.1088/1742-6596/202/1/012033
Citations: PlumX Metrics


2010PI15      Astrophys.J. 710, 1557 (2010)

M.Pignatari, R.Gallino, M.Heil, M.Wiescher, F.Kappeler, F.Herwig, S.Bisterzo

The Weak s-Process in Massive Stars and its Dependence on the Neutron Capture Cross Sections

NUCLEAR REACTIONS 74Ge, 75As, 78Se, 36S, 80Kr(n, γ), E ∼ 30 keV; analyzed available data; deduced Maxwellian averaged σ.

doi: 10.1088/0004-637x/710/2/1557
Citations: PlumX Metrics


2009DI04      Phys.Rev. C 79, 065805 (2009)

I.Dillmann, C.Domingo-Pardo, M.Heil, F.Kappeler, A.Wallner, O.Forstner, R.Golser, W.Kutschera, A.Priller, P.Steier, A.Mengoni, R.Gallino, M.Paul, C.Vockenhuber

Determination of the stellar (n, γ) cross section of 40Ca with accelerator mass spectrometry

NUCLEAR REACTIONS 40Ca(n, γ), E<106 keV; measured σ, σ(E) using activation technique and accelerator mass spectrometry; deduced Maxwellian averaged cross sections. Neutrons from 7Li(p, n)7Be reaction at E(p)=1912 keV. 197Au(n, γ), E<106 keV; measured σ and used as a standard. Comparison with previous experimental data and theoretical predictions.

doi: 10.1103/PhysRevC.79.065805
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset14238.


2009MA35      Phys.Rev. C 79, 065802 (2009)

J.Marganiec, I.Dillmann, C.Domingo Pardo, F.Kappeler, R.Reifarth, R.Gallino, M.Pignatari, P.Grabmayr

Neutron capture cross sections of 74Ge, 76Ge, and 75As at 25 keV

NUCLEAR REACTIONS 74,76Ge, 75As(n, γ), E<106 keV; measured Eγ, Iγ, σ; deduced Maxwellian averaged σ for thermal energies from 5 to 100 keV. Neutrons from 7Li(p, n), E=1912 keV reaction. 197Au(n, γ), E<106 keV; measured σ and used as a standard. Estimated background contributions for γ-ray studies of double β decay of 76Ge.

doi: 10.1103/PhysRevC.79.065802
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset14237.


2009MO10      Phys.Rev. C 79, 045804 (2009)

P.Mohr, S.Bisterzo, R.Gallino, F.Kappeler, U.Kneissl, N.Winckler

Properties of the 5- state at 839 keV in 176Lu and the s-process branching at A=176

NUCLEAR STRUCTURE 176Lu; analyzed partial level scheme, coupling between low- and high-K states; calculated reaction rates for photoactivation process and for transitions from high K ground state to low K isomers in 176Lu. Implications for 176Lu/176Hf as thermometer for astrophysical s-process.

doi: 10.1103/PhysRevC.79.045804
Citations: PlumX Metrics


2008DO05      J.Phys.(London) G35, 014020 (2008)

C.Domingo-Pardo, U.Abbondanno, G.Aerts, H.Alvarez, F.Alvarez-Velarde, S.Andriamonje, J.Andrzejewski, P.Assimakopoulos, L.Audouin, G.Badurek, P.Baumann, F.Becvar, E.Berthoumieux, S.Bisterzo, F.Calvino, M.Calviani, D.Cano-Ott, R.Capote, C.Carrapico, P.Cennini, V.Chepel, N.Colonna, G.Cortes, A.Couture, J.Cox, M.Dahlfors, S.David, I.Dillmann, W.Dridi, I.Duran, C.Eleftheriadis, M.Embid-Segura, L.Ferrant, A.Ferrari, R.Ferreira-Marques, K.Fujii, W.Furman, R.Gallino, I.Goncalves, E.Gonzalez-Romero, F.Gramegna, C.Guerrero, F.Gunsing, B.Haas, R.Haight, M.Heil, A.Herrera-Martinez, M.Igashira, E.Jericha, Y.Kadi, F.Kappeler, D.Karadimos, D.Karamanis, M.Kerveno, P.Koehler, E.Kossionides, M.Krticka, C.Lamboudis, H.Leeb, A.Lindote, I.Lopes, M.Lozano, S.Lukic, J.Marganiec, S.Marrone, C.Massimi, P.Mastinu, A.Mengoni, P.M.Milazzo, M.Mosconi, F.Neves, H.Oberhummer, S.O'Brien, J.Pancin, C.Papachristodoulou, C.Papadopoulos, C.Paradela, N.Patronis, A.Pavlik, P.Pavlopoulos, L.Perrot, M.T.Pigni, R.Plag, A.Plompen, A.Plukis, A.Poch, C.Pretel, J.Quesada, T.Rauscher, R.Reifarth, C.Rubbia, G.Rudolf, P.Rullhusen, J.Salgado, C.Santos, L.Sarchiapone, I.Savvidis, C.Stephan, G.Tagliente, J.L.Tain, L.Tassan-Got, L.Tavora, R.Terlizzi, G.Vannini, P.Vaz, A.Ventura, D.Villamarin, M.C.Vincente, V.Vlachoudis, R.Vlastou, F.Voss, S.Walter, M.Wiescher, K.Wisshak

The measurement of the 206Pb(n, γ) cross section and stellar implications

NUCLEAR REACTIONS 206Pb(n, γ), E=0.001-1000 keV; measured Eγ, Iγ, capture cross sections. Deduced maxwellian averaged sections.

doi: 10.1088/0954-3899/35/1/014020
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22984.


2008HE01      Phys.Rev. C 77, 015808 (2008)

M.Heil, F.Kappeler, E.Uberseder, R.Gallino, M.Pignatari

Neutron capture cross sections for the weak s process in massive stars

NUCLEAR REACTIONS 58Fe, 59Co, 64Ni, 63,65Cu(n, γ), E=25 keV; measured neutron capture cross sections, Eγ; 59Fe, 60Co, 65Ni, 64,66Cu, 198Au; deduced nucleosynthesis yields in stars.

doi: 10.1103/PhysRevC.77.015808
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22996.


2008HE10      Phys.Rev. C 78, 025802 (2008)

M.Heil, F.Kappeler, E.Uberseder, R.Gallino, S.Bisterzo, M.Pignatari

Stellar (n, γ) cross sections for Br and Rb: Matching the weak and main s-process components

NUCLEAR REACTIONS 79,81Br, 85,87Rb(n, γ), E=0-120 keV; measured Eγ, Iγ, σ. 78,80,82Se, 79,81Br, 80,82,83,84,86Kr; 85,87Rb, 86,87,88Sr, 89Y, 90Zr; deduced total s-process abundances.

doi: 10.1103/PhysRevC.78.025802
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset23035.


2008HE17      Astrophys.J. 673, 434 (2008)

M.Heil, N.Winckler, S.Dababneh, F.Kappeler, K.Wisshak, S.Bisterzo, R.Gallino, A.M.Davis, T.Rauscher

176Lu/176Hf: A Sensitive Test of s-Process Temperature and Neutron Density in AGB Stars

NUCLEAR REACTIONS 175Lu(n, γ), E=spectrum; measured Eγ, Iγ, cross sections, isomeric ratio.

doi: 10.1086/523892
Citations: PlumX Metrics


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
Citations: PlumX Metrics


2007HE14      Prog.Part.Nucl.Phys. 59, 174 (2007)

M.Heil, F.Kappeler, E.Uberseder, R.Gallino, M.Pignatari

The s process in massive stars

doi: 10.1016/j.ppnp.2006.12.013
Citations: PlumX Metrics


2007MO01      Phys.Rev. C 75, 012802 (2007)

P.Mohr, F.Kappeler, R.Gallino

Survival of nature's rarest isotope 180Ta under stellar conditions

NUCLEAR REACTIONS 180mTa(γ, γ'), E=low; analyzed σ, T1/2 in stellar environment.

doi: 10.1103/PhysRevC.75.012802
Citations: PlumX Metrics


2007VO02      Phys.Rev. C 75, 015804 (2007)

C.Vockenhuber, I.Dillmann, M.Heil, F.Kappeler, N.Winckler, W.Kutschera, A.Wallner, M.Bichler, S.Dababneh, S.Bisterzo, R.Gallino

Stellar (n, γ) cross sections of 174Hf and radioactive 182Hf

NUCLEAR REACTIONS 174,180,182Hf(n, γ), E=spectrum; measured capture σ; deduced Maxwellian averaged σ, stellar enhancement factors. Comparison with model predictions.

doi: 10.1103/PhysRevC.75.015804
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22963.


2006ST35      Nucl.Phys. A777, 311 (2006)

O.Straniero, R.Gallino, S.Cristallo

s process in low-mass asymptotic giant branch stars

doi: 10.1016/j.nuclphysa.2005.01.011
Citations: PlumX Metrics


2006WA35      Nucl.Phys. A777, 5 (2006)

G.J.Wasserburg, M.Busso, R.Gallino, K.M.Nollett

Short-lived nuclei in the early Solar System: Possible AGB sources

doi: 10.1016/j.nuclphysa.2005.07.015
Citations: PlumX Metrics


2006WI01      Phys.Rev. C 73, 015802 (2006)

K.Wisshak, F.Voss, F.Kappeler, M.Krticka, S.Raman, A.Mengoni, R.Gallino

Stellar neutron capture cross section of the unstable s-process branching point 151Sm

NUCLEAR REACTIONS Sm, 151Sm(n, γ), E=3-225 keV; measured capture σ; deduced Maxwellian averaged σ. Astrophysical implications discussed.

doi: 10.1103/PhysRevC.73.015802
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22916.


2006WI11      Phys.Rev. C 73, 045807 (2006)

K.Wisshak, F.Voss, F.Kappeler, L.Kazakov, F.Becvar, M.Krticka, R.Gallino, M.Pignatari

Fast neutron capture on the Hf isotopes: Cross sections, isomer production, and stellar aspects

NUCLEAR REACTIONS 176,177,178,179,180Hf(n, γ), E=3-225 keV; measured Eγ, Iγ, capture σ; deduced Maxwellian-averaged σ. Astrophysical implications discussed.

doi: 10.1103/PhysRevC.73.045807
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22926.


2006WI20      Astrophys.J. 647, 685 (2006)

N.Winckler, S.Dababneh, M.Heil, F.Kappeler, R.Gallino, M.Pignatari

Lanthanum: An s- and r-Process Indicator

NUCLEAR REACTIONS 139La(n, γ), E=5.1 keV; measured reaction products, Eγ, Iγ; deduced Maxwellian-averaged σ and its uncertainties.

doi: 10.1086/505026
Citations: PlumX Metrics


2005BI19      Nucl.Phys. A758, 284c (2005)

S.Bisterzo, L.Pompeia, R.Gallino, M.Pignatari, K.Cunha, A.Heger, V.Smith

Cu and Zn in different stellar populations: Inferring their astrophysical origin

doi: 10.1016/j.nuclphysa.2005.05.049
Citations: PlumX Metrics


2005CR04      Nucl.Phys. A758, 509c (2005)

S.Cristallo, O.Straniero, R.Gallino

S-process nucleosynthesis in low mass AGB Stars: do we really need an improved determination of the 13C(α, n)16O reaction rate?

doi: 10.1016/j.nuclphysa.2005.05.181
Citations: PlumX Metrics


2005GA39      Nucl.Phys. A758, 485c (2005)

R.Gallino, D.Delaude, L.Husti, S.Cristallo, O.Straniero, S.Ryan

Predictions of s-process Lead in low-metallicity stars compared with spectroscopic observations

doi: 10.1016/j.nuclphysa.2005.05.089
Citations: PlumX Metrics


2005NI17      Nucl.Phys. A758, 348c (2005)

L.R.Nittler, R.Gallino, M.Lugaro, O.Straniero, I.Dominguez, E.Zinner

Si and C Isotopes in Presolar Silicon Carbide Grains From AGB Stars

doi: 10.1016/j.nuclphysa.2005.05.064
Citations: PlumX Metrics


2005PI19      Nucl.Phys. A758, 541c (2005)

M.Pignatari, R.Gallino, F.Kappeler, M.Wiescher

Effects of uncertainties of the 22Ne(α, n)25Mg and 13C(α, n)16O reaction rates in the s-process yields

NUCLEAR REACTIONS 13C, 22Ne(α, n), E=low; analyzed astrophysical reaction rates.

doi: 10.1016/j.nuclphysa.2005.05.098
Citations: PlumX Metrics


2004KA26      Phys.Rev. C 69, 055802 (2004)

F.Kappeler, C.Arlandini, M.Heil, F.Voss, K.Wisshak, R.Reifarth, O.Straniero, R.Gallino, S.Masera, C.Travaglio

Stellar neutron capture on 180Tam. II. Defining the s-process contribution to nature's rarest isotope

NUCLEAR REACTIONS 180mTa(n, γ), E=low; analyzed capture σ; deduced s-process contribution to solar abundance.

doi: 10.1103/PhysRevC.69.055802
Citations: PlumX Metrics


2004PA06      Phys.Rev. C 69, 025803 (2004)

N.Patronis, S.Dababneh, P.A.Assimakopoulos, R.Gallino, M.Heil, F.Kappeler, D.Karamanis, P.E.Koehler, A.Mengoni, R.Plag

Neutron capture studies on unstable 135Cs for nucleosynthesis and transmutation

NUCLEAR REACTIONS 135Cs(n, γ), E=30, 500 keV; measured capture σ. 133,134,135,136,137Cs(n, γ), E=low; deduced Maxwellian averaged σ. Activation technique, comparison with previous results.

RADIOACTIVITY 136Cs(β-) [from 135Cs(n, γ)]; measured T1/2.

doi: 10.1103/PhysRevC.69.025803
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22846.


2004RA29      Phys.Rev. C 70, 065803 (2004)

U.Ratzel, C.Arlandini, F.Kappeler, A.Couture, M.Wiescher, R.Reifarth, R.Gallino, A.Mengoni, C.Travaglio

Nucleosynthesis at the termination point of the s process

NUCLEAR REACTIONS 208Pb, 209Bi(n, γ), E=spectrum; measured σ. Astrophysical implications discussed. Activation technique.

doi: 10.1103/PhysRevC.70.065803
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22883.


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
Citations: PlumX Metrics


2003AR21      Nucl.Phys. A718, 536c (2003)

E.Arnone, R.Gallino, D.L.Lambert, O.Straniero

Nucleosynthesis in FG Sge

doi: 10.1016/S0375-9474(03)00836-4
Citations: PlumX Metrics


2003GA27      Nucl.Phys. A718, 181c (2003)

R.Gallino, E.Arnone, S.Cristallo, S.Masera, C.Travaglio, D.L.Lambert, M.Lugaro, F.Kappeler, H.Van Winckel, M.Reyniers, O.Straniero, A.M.Davis

Minute steps on the quest of the s-process

doi: 10.1016/S0375-9474(03)00711-5
Citations: PlumX Metrics


2003KA50      Nucl.Phys. A718, 173c (2003)

F.Kappeler, A.Mengoni, R.Gallino

Neutron capture studies on difficult isotopes - experiments, theory, and astrophysics

doi: 10.1016/S0375-9474(03)00710-3
Citations: PlumX Metrics


2003LU13      Nucl.Phys. A718, 419c (2003)

M.Lugaro, R.Gallino, S.Amari, E.Zinner, L.R.Nittler

The Effect of Heterogeneities in the Interstellar Medium on the CNO Isotopic Ratios of Presolar SiC and Corundum Grains

doi: 10.1016/S0375-9474(03)00819-4
Citations: PlumX Metrics


2003OB03      Phys.Rev. C 68, 035801 (2003)

S.O'Brien, S.Dababneh, M.Heil, F.Kappeler, R.Plag, R.Reifarth, R.Gallino, M.Pignatari

Neutron capture cross section of 139La

NUCLEAR REACTIONS 139La(n, γ), E=spectrum; measured capture σ; deduced Maxwellian-averaged capture σ. Activation technique. Astrophysical implications discussed.

doi: 10.1103/PhysRevC.68.035801
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22879.


2003RE39      Astrophys.J. 582, 1251 (2003)

R.Reifarth, C.Arlandini, M.Heil, F.Kappeler, P.V.Sedyshev, A.Mengoni, M.Herman, T.Rauscher, R.Gallino, C.Travaglio

Stellar Neutron Capture on Promethium: Implications for the s-Process Neutron Density

NUCLEAR REACTIONS 147Pm(n, γ), E=25 keV; measured reaction products, Eγ, Iγ; deduced Maxwellian-averaged σ and its uncertainties.

NUCLEAR REACTIONS 147,148,149Pm(n, γ), E=5-100 keV; calculated Maxwellian-averaged σ.

COMPILATION 146,147,148Nd, 147,148,149Pm, 147,148,149,150Sm(n, γ), E=10, 25, 30 keV; compiled Maxwellian-averaged σ and its uncertainties.

doi: 10.1086/344718
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22829.


2003SO05      Astrophys.J. 583, 506 (2003)

K.Sonnabend, P.Mohr, K.Vogt, A.Zilges, A.Mengoni, T.Rauscher, H.Beer, F.Kappeler, R.Gallino

The s-Process Branching at 185W

NUCLEAR REACTIONS 186W(γ, n), E=8775 keV bremsstrahlung; measured σ. 186W(γ, n), E=7-10 MeV; calculated σ. 185W(n, γ), E=stellar; calculated Maxwellian averaged σ, astrophysical s-process branching. Activation technique.

doi: 10.1086/345086
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetG0030.


2002RE32      Phys.Rev. C 66, 064603 (2002)

R.Reifarth, M.Heil, F.Kappeler, F.Voss, K.Wisshak, F.Becvar, M.Krticka, R.Gallino, Y.Nagai

Stellar neutron capture cross sections of 128, 129, 130Xe

NUCLEAR REACTIONS 128,129,130Xe(n, γ), E=3-225 keV; measured Eγ, Iγ, capture σ; deduced Maxwellian averaged σ. Astrophysical implications discussed.

doi: 10.1103/PhysRevC.66.064603
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22816.


2001BU21      Nucl.Phys. A688, 505c (2001)

M.Busso, R.Gallino, C.Travaglio, M.Lugaro

s Processing in Post-AGB and CH Stars at Low Metallicity

doi: 10.1016/S0375-9474(01)00770-9
Citations: PlumX Metrics


2001CR05      Nucl.Phys. A688, 217c (2001)

S.Cristallo, O.Straniero, R.Gallino, F.Herwig, A.Chieffi, M.Limongi, M.Busso

The Formation of the 13C Pocket in Asymptotic Giant Branch Stars and Related Nucleosynthesis

doi: 10.1016/S0375-9474(01)00701-1
Citations: PlumX Metrics


2001GA39      Nucl.Phys. A688, 433c (2001)

R.Gallino, C.Travaglio, S.Amari, E.Zinner

Mixing of SN Ejecta with O > C

doi: 10.1016/S0375-9474(01)00747-3
Citations: PlumX Metrics


2001RY03      Nucl.Phys. A688, 209c (2001)

S.G.Ryan, W.Aoki, J.E.Norris, T.C.Beers, R.Gallino, M.Busso, H.Ando

Lead (Pb) in the C-Rich, s-Process Rich, Metal Poor Subgiant LP625-44

doi: 10.1016/S0375-9474(01)00699-6
Citations: PlumX Metrics


2001TR14      Nucl.Phys. A688, 213c (2001)

C.Travaglio, R.Gallino, M.Busso

Galactic Chemical Evolution of Lead: the Role of Asymptotic giant branch stars

doi: 10.1016/S0375-9474(01)00700-X
Citations: PlumX Metrics


2001WI22      Phys.Rev.Lett. 87, 251102 (2001)

K.Wisshak, F.Voss, C.Arlandini, F.Becvar, O.Straniero, R.Gallino, M.Heil, F.Kappeler, M.Krticka, S.Masera, R.Reifarth, C.Travaglio

Neutron Capture on 180Tam: Clue for an s-process origin of nature's rarest isotope

NUCLEAR REACTIONS 180mTa(n, γ), E=10-100 keV; measured capture σ; deduced astrophysical average capture σ.

doi: 10.1103/PhysRevLett.87.251102
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22801.


2001ZI04      Nucl.Phys. A688, 102c (2001)

E.Zinner, S.Amari, R.Gallino, M.Lugaro

Evidence for a Range of Metallicities in the Parent Stars of Presolar SiC Grains

doi: 10.1016/S0375-9474(01)00677-7
Citations: PlumX Metrics


1999AR31      Astrophys.J. 525, 886 (1999)

C.Arlandini, F.Kappeler, K.Wisshak, R.Gallino, M.Lugaro, M.Busso, O.Straniero

Neutron Capture in Low-Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance Signatures

COMPILATION 140,141,142Ce, 141,142Pr, 142,143,144Nd(n, γ); compiled experimental nuclear reaction σ data; deduced sensitive test for models of s-process nucleosynthesis.

doi: 10.1086/307938
Citations: PlumX Metrics


1997BU13      Nucl.Phys. A621, 431c (1997)

M.Busso, R.Gallino

s-Process Abundances in AGB Stars at Various Metallicities and Their Theoretical Interpretation

doi: 10.1016/S0375-9474(97)00285-6
Citations: PlumX Metrics


1997GA19      Nucl.Phys. A621, 423c (1997)

R.Gallino, C.Arlandini, M.Lugaro, M.Busso, O.Straniero

The New s-Process in Low Mass TP-AGB Stars

doi: 10.1016/S0375-9474(97)00284-4
Citations: PlumX Metrics


1993RA24      Astrophys.J. 419, 207 (1993)

C.M.Raiteri, R.Gallino, M.Busso, D.Neuberger, F.Kappeler

The Weak s-Component and Nucleosynthesis in Massive Stars

NUCLEAR REACTIONS 87Rb(n, γ), E=25, 30 keV; measured reaction products, Eγ, Iγ; deduced Maxwellian-averaged σ and its uncertainties.

COMPILATION 58,59,60Fe, 59,60Co, 58,59,60,61,62,63,64Ni, 63,64,65Cu, 64,65,66,67,68,70Zn, 69,71Ga, 70,71,72,73,74,76Ge, 75As, 76,77,78,79,80,82Se, 79,80,81Br, 80,81,82,83,84,85,86Kr, 85,86,87Rb, 86,87,88,89,90Sr, 89,90Y, 90,91,92,93,94,96Zr(n, γ), E=26, 91 keV; compiled experimental and theoretical (n, γ) Maxwellian-averaged σ and their uncertainties.

doi: 10.1086/173476
Citations: PlumX Metrics


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