Chemical evolution of bulges and halos

Details Chemical evolution of bulges and halos Chemical evolution of bulges and halos

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..773m&link_type=abstract

(Astronomical Society of the Pacific, Symposium on Stellar Populations, University of California, Santa Cruz, CA, July 9-12, 198

Other

52

Chemical Evolution, Galactic Evolution, Globular Clusters, Interstellar Chemistry, Metallicity, Astronomical Models, Colorimetry, Elliptical Galaxies, Galactic Structure, Halos, Mass Distribution, Spiral Galaxies

Scientific paper

The chemical properties of elliptical galaxies and the bulges of spiral galaxies are reviewed. The mass-metallicity relation for ellipticals appears to span the full range of these galaxies from dwarf spheroidal to gE. Explanations seem possible in terms of galaxy formation models with dissipation and mass loss, but other solutions such as variable yield are discussed. The properties of globular cluster systems and their "parent" galaxies are compared.

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