Halo Star Abundances and r-Process Synthesis
classification
🌌 astro-ph
keywords
abundanceschemicalearlyelementevolutionexploregalactichalo
read the original abstract
We review recent observational studies of heavy element abundances in low metallicity stars and explore some implications of these results for nucleosynthesis and early Galactic chemical evolution.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.