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Lyman-alpha clouds as a relic of primordial density fluctuations

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/165923· OSTI ID:5339104
Primordial density fluctuations are studied using a CDM model and primordial clouds some of which are expanding, driven by pressure gradients created when the medium is photionized, and some of which are massive enough to continue collapsing in spite of the pressure. Normalization of CDM models to the clustering properties on large scales are used to predict the parameters of collapsing clouds of subgalactic mass at early epochs. It is shown that the abundance and dimensions of these clouds are comparable to those of the Lyman-alpha systems. The evolutionary history of the clouds is computed, utilizing a spherically symmetric hydrodynamics code with the dark matter treated as a collisionless fluid, and the H I column density distribution is evaluated as a function of N(H I) and redshift. The observed cloud parameters come out naturally in the CDM model and suggest that Lyman-alpha clouds are the missing link between primordial density fluctuations and the formation of galaxies. 31 references.
Research Organization:
Toronto Univ. (Canada); NASA/Fermi National Accelerator Laboratory, Batavia, IL (USA); Eotvos Lorand Tudomanyeyetem, Budapest (Hungary); California Univ., Berkeley (USA)
OSTI ID:
5339104
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 324; ISSN ASJOA
Country of Publication:
United States
Language:
English