Electronic Resource
Springer
Astrophysics and space science
265 (1999), S. 355-359
ISSN:
1572-946X
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
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.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1023/A:1002101003660
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