The chemical evolution of elliptical galaxies

Details The chemical evolution of elliptical galaxies The chemical evolution of elliptical galaxies

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...236..754h&link_type=abstract

Astrophysical Journal, Part 1, vol. 236, Mar. 15, 1980, p. 754-760.

Astronomy and Astrophysics

Astrophysics

11

Chemical Evolution, Elliptical Galaxies, Galactic Evolution, Globular Clusters, Star Distribution, Visual Photometry, Abundance, Astronomical Models, Astronomical Photometry, Hertzsprung-Russell Diagram, Interstellar Matter, Metals

Scientific paper

U-R colors of elliptical and S0 galaxies have been synthesized by combining the stellar populations of galactic globular clusters in accordance with a simple mass-loss chemical evolutionary model. The model independently predicts the mass and metal abundance of the intracluster medium, which agrees with recent model dependent interpretations of the X-ray observations of clusters of galaxies.

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