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Paper: Neutron-Capture Nucleosynthesis in AGB Stars and their Connection with Dwarf Spheroidal Galaxies and the Galactic Halo
Volume: 458, Galactic Archaeology: Near-Field Cosmology and the Formation of the Milky Way
Page: 41
Authors: Fishlock, C. K.; Karakas, A. I.; Yong, D.
Abstract: Using a sample of Galactic halo stars, we will investigate two distinct Galactic halo populations separated by [α/Fe]. The low-α population may be the result of accretion from a dwarf galaxy. Some dwarf galaxies show the signature of asymptotic giant branch (AGB) nucleosynthesis through their neutron-capture element abundance distribution. AGB stars are a known site for the production of heavy elements via the slow neutron-capture process (the s-process). We aim to calculate yields of s-process elements from AGB models. These yields will be used as input into a chemical evolution model for comparison to the high-resolution Magellan data obtained for this investigation.
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