Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S344(14), p. 220-221, 2018
DOI: 10.1017/s174392131800529x
Full text: Unavailable
AbstractWe analyse the chemical abundances of stars in the local group dwarf galaxies using the SAGA database. The inspection of the relationship between Eu and Ba abundances confirms an anomalously Ba-rich population in Fornax, which indicates a pre-enrichment of interstellar gas with r-process elements.