Formation and development of elliptical and dwarf galaxies

Details Formation and development of elliptical and dwarf galaxies Formation and development of elliptical and dwarf galaxies

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phdt........19b&link_type=abstract

Ph.D. Thesis Ludwig-Maximilians-Univ., Munich (Germany, F.R.). Fakultaet für Physik.

Mathematics

7

Astronomical Models, Dwarf Galaxies, Elliptical Galaxies, Stellar Evolution, Stellar Systems, Analysis (Mathematics), Dissipation, Gas-Solid Interactions, Growth, Interstellar Matter

Scientific paper

A consistent model for the formation and development of elliptical and dwarf galaxies is presented. The observed global properties of these galaxies were examined. As galaxies in the late phase of their development are mostly composed of stars, the dynamics of stellar systems plays an important part in the galaxy development. The development of stellar systems was examined, and the results are discussed, using a new star dynamics model. It was found that the development of stellar systems strongly depends on the collapse of this system. A detailed Inter Stellar Medium (ISM) model was presented. The interaction process between the star components and the gas components was determined. Using this ISM model, the chemidynamical development of the elliptical and dwarf galaxies was analytically and numerically examined.

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