Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
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F 60 e Anomaly in a Deep-Sea Manganese Crust and Implications for a Nearby Supernova SourceNeutron capture cross section of unstable 63Ni: implications for stellar nucleosynthesisThe evolution of the Milky Way from its earliest phases: Constraints on stellar nucleosynthesisShort-lived chlorine-36 in a Ca- and Al-rich inclusion from the Ningqiang carbonaceous chondrite.Phosphorus in the young supernova remnant Cassiopeia A.Stardust in meteoritesRecent near-Earth supernovae probed by global deposition of interstellar radioactive (60)Fe.Origin of the p-process radionuclides 92Nb and 146Sm in the early solar system and inferences on the birth of the SunAb initio alpha-alpha scattering.The locations of recent supernovae near the Sun from modelling (60)Fe transport.Early solar system. Stellar origin of the ¹⁸²Hf cosmochronometer and the presolar history of solar system matter.Effective helium burning rates and the production of the neutrino nuclei.Solution of the α-potential mystery in the γ process and its impact on the Nd/Sm ratio in meteorites.Interstellar ^{60}Fe on the Surface of the Moon.Stardust in Antarctic micrometeoritesSystematic study of (p,γ) reactions on Ni isotopesAstrophysical analysis of the measurement of (α,γ) and (α,n) cross sections of169TmPerspectives for photonuclear research at the Extreme Light Infrastructure - Nuclear Physics (ELI-NP) facilityEssential ingredients in core-collapse supernovaeMeasurement of the24Mg(3He,p)26Alcross section: Implication forAl26production in the early solar systemE1andE2Sfactors ofC12(α,γ0)O16fromγ-ray angular distributions with a 4π-detector arrayNi62(n,γ) and Ni63(n,γ) cross sections measured at the n_TOF facility at CERNInvestigation of the reaction74Ge(p,γ)75As using the in-beam method to improve reaction network predictions forpnucleiCross section measurements of theY89(p,γ)Zr90reaction at energies relevant top-process nucleosynthesisConvective overshooting and production of s-nuclei in massive stars during their core He-burning phaseMultimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and ObservationMeasurement of theRe187(α,n)Ir190reaction cross section at sub-Coulomb energies using the Cologne Clover Counting SetupDetermination of141Pr(α,n)144Pm cross sections at energies of relevance for the astrophysicalpprocess using theγγcoincidence methodChemodynamical Simulations of Dwarf Galaxy EvolutionRadioactive 26Al from massive stars in the Galaxy
P2860
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P2860
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im September 2002 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 2002
@uk
name
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
@en
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
@nl
type
label
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
@en
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
@nl
prefLabel
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
@en
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
@nl
P2093
P356
P1476
Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics
@en
P2093
R. D. Hoffman
S. E. Woosley
P304
P356
10.1086/341728
P407
P577
2002-09-01T00:00:00Z
P5875
P818
astro-ph/0112478
P819
2002ApJ...576..323R