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Biased Galaxy Formation and Dark Matter
Published online by Cambridge University Press: 03 August 2017
Abstract
The clustering properties of galaxies are incompatible with a cosmological model with Ω = 1 unless the formation process for bright galaxies is ‘biased’ in the sense that their resultant distribution exaggerates the amplitude of large-scale inhomogeneities in the overall mass distribution. The mechanisms for such biasing are intimately connected with the nature of the dark matter. Various possibilities are summarised here.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 437 - 446
- Copyright
- Copyright © Reidel 1988