Origin of metals in old Milky Way halo stars based on GALAH and Gaia

Author(s):
Ishigaki, M.N.; Hartwig, T.; Tarumi, Y.; Leung, S.C.; Tominaga, N.; Kobayashi, C.; Magg, M.; Simionescu, A.; Nomoto, K.
Published
2021
Publication type
Article / Letter to editor
Nuclear reactionsNucleosynthesisAbundancesStars: abundancesStars: fundamental parametersStars: kinematics and dynamicsStars: Population IIISupernovae: generalAstrophysics - astrophysics of galaxies
Date issued
2021
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2021), Vol. 506, no. 4, p. 5410-5429
hdl
1887/3275502
doi
10.1093/mnras/stab1982
URL
https://ui.adsabs.harvard.edu/abs/2021MNRAS.506.5410I