Using neutron-capture abundances as a tracer of Galactic halo formation
Date
2013
Authors
Fishlock, Cherie
Karakas, Amanda
Lugaro, Maria
Yong, David
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Conference Organising Committee
Abstract
Chemical differences in stellar populations are one method to study the formation and evolution of the Galactic halo of the Milky Way. In particular, there are low α-element stars and high α-element stars in the Galactic halo that also show differences
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Source
Proceedings of Science
Type
Conference paper
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Restricted until
2037-12-31