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| 001 | 364050 | ||
| 005 | 20260113232406.0 | ||
| 024 | 7 | _ | |a 10.5281/ZENODO.15765631 |2 doi |
| 037 | _ | _ | |a GSI-2026-00232 |
| 041 | _ | _ | |a English |
| 100 | 1 | _ | |a Thielemann, Friedrich-Karl |0 P:(DE-Ds200)OR3007 |b 0 |u gsi |
| 111 | 2 | _ | |a VLT, SUPERNOVAE, BRUNO |c Garching |d 2025-01-07 - 2025-01-11 |w Germany |
| 245 | _ | _ | |a Clues on the (supernovae or non-supernovae) Origins of the Elements from Galactic Archeology |
| 260 | _ | _ | |c 2025 |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a Other |2 DataCite |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 336 | 7 | _ | |a conferenceObject |2 DRIVER |
| 336 | 7 | _ | |a LECTURE_SPEECH |2 ORCID |
| 336 | 7 | _ | |a Conference Presentation |b conf |m conf |0 PUB:(DE-HGF)6 |s 1768309109_1480590 |2 PUB:(DE-HGF) |x Other |
| 500 | _ | _ | |a Creative Commons Attribution 4.0 International |
| 520 | _ | _ | |a 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] |
| 536 | _ | _ | |a 612 - Cosmic Matter in the Laboratory (POF4-612) |0 G:(DE-HGF)POF4-612 |c POF4-612 |f POF IV |x 0 |
| 588 | _ | _ | |a Dataset connected to DataCite |
| 693 | _ | _ | |a theory |e no experiment theory work (theory) |1 EXP:(DE-Ds200)theory-20200803 |0 EXP:(DE-Ds200)no_experiment-20200803 |5 EXP:(DE-Ds200)no_experiment-20200803 |x 0 |
| 773 | _ | _ | |a 10.5281/ZENODO.15765631 |
| 909 | C | O | |o oai:repository.gsi.de:364050 |p VDB |
| 910 | 1 | _ | |a GSI Helmholtzzentrum für Schwerionenforschung GmbH |0 I:(DE-Ds200)20121206GSI |k GSI |b 0 |6 P:(DE-Ds200)OR3007 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Matter and the Universe |1 G:(DE-HGF)POF4-610 |0 G:(DE-HGF)POF4-612 |3 G:(DE-HGF)POF4 |2 G:(DE-HGF)POF4-600 |4 G:(DE-HGF)POF |v Cosmic Matter in the Laboratory |x 0 |
| 914 | 1 | _ | |y 2025 |
| 920 | 1 | _ | |0 I:(DE-Ds200)KNA-20160901OR396 |k KNA |l Nukleare Astrophysik & Struktur |x 0 |
| 980 | _ | _ | |a conf |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a I:(DE-Ds200)KNA-20160901OR396 |
| 980 | _ | _ | |a UNRESTRICTED |
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