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The Clustering of QSO Absorption-Line Systems

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dc.contributor.authorFrancis, Paul
dc.contributor.authorVeeraraghavan, Shoba
dc.date.accessioned2018-10-02T06:42:00Z
dc.date.available2018-10-02T06:42:00Z
dc.date.issued1995
dc.description.abstractA growing body of mainly anecdotal evidence suggests that, at high redshifts, metal-line and damped Lyman-α absorption-line systems cluster very strongly, perhaps more strongly than bright galaxies today! We review this evidence, and present first results from a complete, quantitative survey of absorption-line clustering. We detect clustering of high column-density Lyman-α lines and C IV systems, and place an upper limit on the clustering of Mg II systems.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.isbn978-3-662-22373-4en_AU
dc.identifier.issn1431-2433en_AU
dc.identifier.urihttp://hdl.handle.net/1885/148006
dc.publisherSpringer Verlagen_AU
dc.rights© Springer-Verlag Berlin Heidelberg 1995en_AU
dc.subjectAnecdotal Evidenceen_AU
dc.subjectGalaxy Clusteren_AU
dc.subjectHigh Redshiften_AU
dc.subjectQuantitative Surveyen_AU
dc.subjectFluctuation Amplitudeen_AU
dc.titleThe Clustering of QSO Absorption-Line Systemsen_AU
dc.typeConference paperen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.lastpage362en_AU
local.bibliographicCitation.startpage361en_AU
local.contributor.affiliationFrancis, P., Mount Stromlo Observatory, Research School of Astronomy and Astrophysics, The Australian National Universityen_AU
local.contributor.authoruidu9710753en_AU
local.identifier.doi10.1007/978-3-540-49458-4_75en_AU
local.publisher.urlhttps://link.springer.comen_AU
local.type.statusPublished Versionen_AU

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