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87th Annual Meeting of the Meteoritical Society 2025: Contents
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 2-29, August 2025.
wiley +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Underground nuclear astrophysics studies with CASPAR
The drive of low-energy nuclear astrophysics laboratories is to study the reactions of importance to stellar burning processes and elemental production through stellar nucleosynthesis, over the energy range of astrophysical interest.
Robertson Daniel +4 more
doaj +1 more source
The merger between the carbon (C) and oxygen (O) shells hours to days before the collapse of a massive star significantly changes its nucleosynthesis, which is reflected in the elemental ratios observed in supernova remnants (SNRs).
L. Boccioli +5 more
doaj +1 more source
Editorial: Nuclear Reactions of Astrophysical Interest
Scilla Degl’Innocenti +4 more
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Physical Conditions for Synthesis of Sc, Ti, and V in Neutrino-driven Supernovae
We present the results of simulations of nucleosynthesis in a core-collapse supernova including the neutrino process. Using the Si layer of a 13 M _⊙ zero-metal progenitor as the initial composition, we calculate the nucleosynthesis by adopting the ...
Ryota Hatami +4 more
doaj +1 more source
The Impact of Recent LUNA Measurements of NeNa Reactions on 26Al Stellar Nucleosynthesis
Recent measurements performed by the LUNA(Laboratory for Underground Nuclear Astrophysics) collaboration between 2019 and 2024 have provided the most precise direct determinations to date of several key reaction rates in the NeNa cycle, specifically the ...
Umberto Battino +8 more
doaj +1 more source
Measuring neutron capture cross sections of radioactive nuclei: From activations at the FZK Van de Graaff to direct neutron captures in inverse kinematics with a storage ring at TRIUMF. [PDF]
Dillmann I +10 more
europepmc +1 more source
Detection of Metal Enrichment by SN 2011jm in NGC 4809
Cosmic metals are believed to originate from stellar and supernovae (SNe) nucleosynthesis, dispersed into the interstellar medium (ISM) through stellar winds and supernova explosions.
Yulong Gao +4 more
doaj +1 more source
A metal-poor star with abundances from a pair-instability supernova. [PDF]
Xing QF +9 more
europepmc +1 more source

