A chemical abundance analysis of stars believed to be metal poor members of the galactic stellar thick disk
Galactic formation models have long sought to reproduce the observed chemical and kinematical properties of the Milky Way's stellar halo and disk. Recently it is the so-called "intermediate population", the stellar thick disk, that is driving advances in our understanding of the forma...
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| Format: | Others |
| Language: | English |
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2015
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| Online Access: | http://hdl.handle.net/2152/29671 |