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- W1649670069 abstract "Investigations of the structure and evolution of the Galaxy have been restricted strongly to the study of nearby stellar samples, supplemented by relatively meager distant in situ ones. The advent of wide field spectroscopic facilities opens the way to the investigation of statistically meaningful distant samples which will make it possible to provide solutions to such questions as the role of the minority halo and thick disk populations, the disentangling of the populations in the Galactic bulge, the accretion of material to the Galaxy, and the determination of the total mass of the system, and thereby provide strong constraints not only on its present structure, but also on the manner in which it formed and has evolved." @default.
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- W1649670069 date "1997-01-01" @default.
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- W1649670069 title "Wide Field Spectroscopy & the Structure of the Galaxy" @default.
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- W1649670069 doi "https://doi.org/10.1007/978-94-011-5722-3_23" @default.
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