364050 20260113232406.0 10.5281/ZENODO.15765631 doi GSI-2026-00232 English Thielemann, Friedrich-Karl P:(DE-Ds200)OR3007 0 gsi VLT, SUPERNOVAE, BRUNO Garching 2025-01-07 - 2025-01-11 Germany Clues on the (supernovae or non-supernovae) Origins of the Elements from Galactic Archeology 2025 Conference Paper 33 EndNote Other DataCite INPROCEEDINGS BibTeX conferenceObject DRIVER LECTURE_SPEECH ORCID Conference Presentation conf conf PUB:(DE-HGF)6 1768309109_1480590 PUB:(DE-HGF) Other Creative Commons Attribution 4.0 International Low-metallicity stars are witnesses of the first stellar nucleosynthesis events in the Galaxy, as their surface abundances reflect the composition of the interstellar medium from which they were born. Aside from the primordial Big Bang nucleosynthesis, massive stars, due to their short lifetimes, dominate the wind and explosive ejecta into the interstellar medium of the early Galaxy. Most of them will end as core-collapse supernova (CCSN) explosions, and typical abundance patterns reflect their influence. Essentially all CCSNe eject Fe (decaying from radioactive 56Ni). Therefore, it is interesting to test whether other elements found in low-metallicity stars are correlated with Fe, i.e. whether they have been co-produced in the contributing sources or require either different or additional astrophysical origins. We concentrate in our analysis on stars with [Fe/H] 612 - Cosmic Matter in the Laboratory (POF4-612) G:(DE-HGF)POF4-612 POF4-612 POF IV 0 Dataset connected to DataCite theory no experiment theory work (theory) EXP:(DE-Ds200)theory-20200803 EXP:(DE-Ds200)no_experiment-20200803 EXP:(DE-Ds200)no_experiment-20200803 0 10.5281/ZENODO.15765631 oai:repository.gsi.de:364050 VDB GSI Helmholtzzentrum für Schwerionenforschung GmbH I:(DE-Ds200)20121206GSI GSI 0 P:(DE-Ds200)OR3007 DE-HGF Forschungsbereich Materie Matter and the Universe G:(DE-HGF)POF4-610 G:(DE-HGF)POF4-612 G:(DE-HGF)POF4 G:(DE-HGF)POF4-600 G:(DE-HGF)POF Cosmic Matter in the Laboratory 0 2025 I:(DE-Ds200)KNA-20160901OR396 KNA Nukleare Astrophysik & Struktur 0 conf VDB I:(DE-Ds200)KNA-20160901OR396 UNRESTRICTED