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dc.contributor.authorGardner, J. P.
dc.contributor.authorKatz, N.
dc.contributor.authorHernquist, L.
dc.contributor.authorWeinberg, D. H.
dc.date.accessioned2019-09-20T10:34:38Z
dc.date.issued2001
dc.identifier.citationGardner, Jeffrey P., Neal Katz, Lars Hernquist, and David H. Weinberg. 2001. “Simulations of Damped Lyα and Lyman Limit Absorbers in Different Cosmologies: Implications for Structure Formation at High Redshift.” The Astrophysical Journal 559 (1): 131–46. https://doi.org/10.1086/322403.
dc.identifier.issn0004-637X
dc.identifier.issn1538-4357
dc.identifier.urihttp://nrs.harvard.edu/urn-3:HUL.InstRepos:41381835*
dc.description.abstractWe use hydrodynamic cosmological simulations to study damped Ly alpha (DLA) and Lyman limit (LL) absorption at redshifts z = 2-4 in five variants of the cold dark matter scenario: COBE-normalized (CCDM), cluster-normalized (SCDM), and tilted (n = 0.8) Omega (m) = 1 models, as well as open (OCDM) and flat (LCDM) Omega (m) = 0.4 models. Our standard simulations resolve the formation of dense concentrations of neutral gas in halos with circular velocity v
dc.language.isoen_US
dc.publisherAmerican Astronomical Society
dash.licenseLAA
dc.titleSimulations of damped Ly alpha and Lyman limit absorbers in different cosmologies: Implications for structure formation at high redshift
dc.typeJournal Article
dc.description.versionAccepted Manuscript
dc.relation.journalThe Astrophysical Journal
dash.depositing.authorHernquist, Lars Eric::39d9dfe7535406d002e4507056194fd1::600
dc.date.available2019-09-20T10:34:38Z
dash.workflow.comments1Science Serial ID 96091
dc.identifier.doi10.1086/322403
dash.source.volume559;1


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