Globular Clusters and field stars in the Bulge |
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Authors: | S Ortolani |
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Institution: | (1) Department of Astronomy, University of Padova, Vicolo dell'Osservatorio 5, Padova, I-35122, Italy |
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Abstract: | In this paper we discuss the characteristics of the stellar content of the galactic bulge excluding the stars within a few
parsec from the galactic center. The bulge clusters and the field stars are comparedto the disk population. A scenario with
a flattened bulge extending toabout 3–4 Kpc from the galactic center is presented. There is evidencefor an old bulge stellar
population, decoupled from the disk.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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Keywords: | |
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