% IMPORTANT: The following is UTF-8 encoded. This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.
@INPROCEEDINGS{Thielemann:364050,
author = {Thielemann, Friedrich-Karl},
title = {{C}lues on the (supernovae or non-supernovae) {O}rigins of
the {E}lements from {G}alactic {A}rcheology},
reportid = {GSI-2026-00232},
year = {2025},
note = {Creative Commons Attribution 4.0 International},
abstract = {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]},
month = {Jan},
date = {2025-01-07},
organization = {VLT, SUPERNOVAE, BRUNO, Garching
(Germany), 7 Jan 2025 - 11 Jan 2025},
subtyp = {Other},
cin = {KNA},
cid = {I:(DE-Ds200)KNA-20160901OR396},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612)},
pid = {G:(DE-HGF)POF4-612},
experiment = {$EXP:(DE-Ds200)no_experiment-20200803$},
typ = {PUB:(DE-HGF)6},
doi = {10.5281/ZENODO.15765631},
url = {https://repository.gsi.de/record/364050},
}