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What are the implications of stellar chemical abundances in dwarf galaxies?
Published online by Cambridge University Press: 30 October 2019
Abstract
We 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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 14 , Symposium S344: Dwarf Galaxies: From the Deep Universe to the Present , August 2018 , pp. 220 - 221
- Copyright
- © International Astronomical Union 2019