Title: New limits to bias and the amount of dark matter in the universe
Abstract: view Abstract Citations (9) References (20) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS New Limits to Bias and the Amount of Dark Matter in the Universe Saslaw, William C. ; Antia, H. M. ; Chitre, S. M. Abstract The observed thermodynamic distribution function f(N) for galaxies places significant constraints on the amount of structured dark matter in the universe. The simplest models of cold dark matter require the cosmological density parameter Ω0 ⪉ 0.4. Biased galaxy formation in more complicated models must have specific forms which depend on the amount and structure of dark matter in the model. Publication: The Astrophysical Journal Pub Date: April 1987 DOI: 10.1086/184850 Bibcode: 1987ApJ...315L...1S Keywords: Cosmology; Dark Matter; Galactic Clusters; Galactic Evolution; Astronomical Models; Distribution Functions; Statistical Distributions; Astrophysics; COSMOLOGY; GALAXIES: CLUSTERING; GALAXIES: FORMATION full text sources ADS |
Publication Year: 1987
Publication Date: 1987-04-01
Language: en
Type: article
Indexed In: ['crossref']
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Cited By Count: 10
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