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The Evolutionary History of the Milky Way
Published online by Cambridge University Press: 25 May 2016
Abstract
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The accretion of small satellite galaxies appears to have been important in the formation of the metal-poor halo of the Galaxy. The disrupting Sgr dwarf galaxy and the recent discovery of a young, metal-poor component of the halo indicate that this is a continuing process. The evolution of the galactic disk, and some consequences of the bar-like nature of the galactic bulge are briefly discussed.
- Type
- Spiral Galaxies
- Information
- Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 3 - 10
- Copyright
- Copyright © Kluwer 1996
References
de Vaucouleurs, G.
1964. In “The Galaxy and the Magellanic Clouds” (Austr. Acad. Sci), ed. Kerr, F. and Rodgers, A., p 195.Google Scholar
Gerhard, O.
1995. In “Unsolved Problems of the Milky Way” (Kluwer), ed Blitz, L., in press.Google Scholar
Toomre, A.
1977. In “The Evolution of Galaxies and Stellar Populations” (Yale University Observatory), ed Tinsley, B. and Larson, R., p 420.Google Scholar
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