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THE HISTORY OFR-PROCESS ENRICHMENT IN THE MILKY WAY
2015
Astrophysical Journal
We investigate the production sites and the enrichment history of r-process elements in the Galaxy, as traced by the [Eu/Fe] ratio, using the high resolution, cosmological zoom-in simulation 'Eris'. At z=0, Eris represents a close analog to the Milky Way, making it the ideal laboratory to understand the chemical evolution of our Galaxy. Eris formally traces the production of oxygen and iron due to Type-Ia and Type-II supernovae. We include in post-processing the production of r-process elements
doi:10.1088/0004-637x/807/2/115
fatcat:inhjnxglojht3b4gvitovtjs4e