Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aj....104..144w&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 104, no. 1, July 1992, p. 144-153.
Astronomy and Astrophysics
Astronomy
110
Astronomical Models, Galactic Bulge, Galactic Evolution, Spheroids, Star Formation, Abundance, Angular Momentum, Hydrogen, Iron, Metallic Stars, Stellar Mass, Supernovae
Scientific paper
Several possible models for the evolution of the Galactic r exp 1/4 spheroid and bulge are discussed, with special attention given to the fate of the missing spheroid mass and the rate of star formation in the bulge. Attention is called to a possibility that the spheroid is chemically distinct from the disk and that the spheroid gas fell toward the center of the Galaxy and formed the central bulge, as suggested by angualr momentum considerations.
Gilmore Gerard
~Wyse Rosemary F. G.
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