Formation of galaxies

Details Formation of galaxies Formation of galaxies

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984stin...8529863s&link_type=abstract

Presented at Intern. Symp. on Phase Transitions in the Very Early Universe, Rielefeld, West Germany, 1 Jun. 1984

Physics

Correlation Coefficients, Cosmology, Galactic Clusters, Galactic Evolution, Galactic Structure, Red Shift, Baryons, Lyman Alpha Radiation, Particle Interactions, Theoretical Physics

Scientific paper

The present theories of galaxy formation are reviewed. The relation between peculiar velocities and the correlation function of galaxies points to the possibility that galaxies do not form uniformly everywhere. Scale invariant properties of the cluster-cluster correlations are discussed. Comparing the correlation functions in a dimensionless way, galaxies appear to be stronger clustered, in contrast with the comparison of the dimensional amplitudes of the correlation functions. Theoretical implications of several observations as Lyman-(ALPHA) clouds, correlations of faint galaxies are discussed. None of the present theories of galaxy formation can account for all facts in a natural way.

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