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Galaxy Formation and Evolution: What to Expect from Hierarchical Clustering Models

Published online by Cambridge University Press:  25 May 2016

C.S. Frenk ,
C.M. Baugh  and
S. Cole
C.S. Frenk
Affiliation:
Physics Department, University of Durham, UK
C.M. Baugh
Affiliation:
Physics Department, University of Durham, UK
S. Cole
Affiliation:
Physics Department, University of Durham, UK

Extract

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In hierarchical clustering theories of galaxy formation, galaxies form by gas cooling and condensing into dark matter halos which, in turn, form by a hierarchy of mergers (White & Rees 1978). The context in which this process takes place is specified by a cosmological model that determines the spectrum of primordial density fluctuations and the rate at which they grow by gravitational instability. The best known example of such a model is the cold dark matter (CDM) model (see Frenk 1991 for a review), but a number of alternatives (mostly variants of CDM), have recently become popular in response to new data on large-scale structure and the COBE detection of anisotropies in the microwave background radiation.

Type
Theory of Galaxy Formation
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 247 - 254
Copyright
Copyright © Kluwer 1996 

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