Models of the evolution of star formation regions in blue compact dwarf galaxies. II - Chemical evolution

Details Models of the evolution of star formation regions in blue compact dwarf galaxies. II - Chemical evolution Models of the evolution of star formation regions in blue compact dwarf galaxies. II - Chemical evolution

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...77p&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, May-June 1991, p. 77-81. In Russian.

Computer Science

Chemical Evolution, Compact Galaxies, Dwarf Galaxies, Star Formation, Stellar Evolution, Abundance, Hydrogen Ions, Interstellar Gas, Stellar Composition, Stellar Mass

Scientific paper

The chemical evolution of star formation regions in blue compact dwarf galaxies is considered. It is shown that the chemical composition of these regions varies substantially in their evolution process. The gas density and initial mass function of the star formation burst are the main factors which determine the change of metal abundances in the star formation region.

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