Spatial structure of protoclusters and the formation of galaxies

Details Spatial structure of protoclusters and the formation of galaxies Spatial structure of protoclusters and the formation of galaxies

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184..643d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 184, Sept. 1978, p. 643-660.

Astronomy and Astrophysics

Astronomy

80

Astronomical Models, Galactic Clusters, Galactic Evolution, Galactic Structure, Adiabatic Conditions, Gas Dynamics, Gravity Anomalies, Interstellar Gas, Nonlinear Systems, Pressure Effects, Shock Fronts, Thermodynamics, Three Dimensional Models

Scientific paper

Three-dimensional models of 'pancakes' are constructed and their temporal evolution is followed. It is shown that in the course of evolution thermal, hydrodynamic and gravitational instabilities arise which lead to the fragmentation of gaseous protoclusters and the subsequent clustering of fragments into galaxies and clusters of galaxies. This scheme is shown to explain a number of observational facts.

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