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Investigation of ancient substructures in the Milky Way: chemical composition study
Published online by Cambridge University Press: 09 March 2010
Abstract
From high resolution spectra taken with the spectrograph FIES on the Nordic Optical Telescope, La Palma, we measure abundances of oxygen and α-elements in order to characterize stars which from their dynamical properties are suspected to have originated in disrupted satellites. We find that the chemical composition of investigated stars is homogeneous and distinct from Galactic disk dwarfs, which is providing further evidence of their extragalactic origin.
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- Copyright © International Astronomical Union 2010