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.
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Ortolani, S. Globular Clusters and field stars in the Bulge. Astrophysics and Space Science 265, 355–359 (1999). https://doi.org/10.1023/A:1002101003660
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DOI: https://doi.org/10.1023/A:1002101003660