Chemical evolution of the members of the Local Group

Details Chemical evolution of the members of the Local Group Chemical evolution of the members of the Local Group

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mmsai..50...11v&link_type=abstract

(Workshop on Chemical Inhomogeneities in the Galaxy, Frascati, Italy, May 29-June 2, 1978.) Società Astronomica Italiana, Memori

Astronomy and Astrophysics

Astronomy

3

Abundance, Chemical Evolution, Galactic Clusters, Galactic Evolution, Interstellar Chemistry, Local Group (Astronomy), Magellanic Clouds, Milky Way Galaxy

Scientific paper

An examination of data on the chemical evolution of the Local Group shows that the chemical abundance of the galaxies involved appears to be determined mainly by galaxy mass. Color/magnitude diagrams of clusters suggest that the Fe/CNO ratio may differ between disks and halos of galaxies. Another important parameter is variations in the C/O abundance ratio.

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