Clustering of Absorbers

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dc.creatorCristiani, S.
dc.creatorD'Odorico, S.
dc.creatorD'Odorico, V.
dc.creatorFontana, A.
dc.creatorGiallongo, E.
dc.creatorMoscardini, L.
dc.creatorSavaglio, S.
dc.date1997-11-14
dc.date.accessioned2026-07-07T02:25:05Z
dc.date.available2026-07-07T02:25:05Z
dc.descriptionThe observed clustering of Lyman-$α$ lines is reviewed and compared with the clustering of CIV systems. We argue that a continuity of properties exists between Lyman-$α$ and metal systems and show that the small-scale clustering of the absorbers is consistent with a scenario of gravitationally induced correlations. At large scales statistically significant over and under-densities (including voids) are found on scales of tens of Mpc.
dc.description8 pages Latex, with 2 PostScript figures, using conf_iap.sty. To appear in the Proceedings of the 13th IAP (Paris) Colloquium (July 1-5, 1997) Structure and Evolution of the IGM from QSO Absorption Line Systems, eds. P.Petitjean, S.Charlot
dc.identifierhttps://arxiv.org/abs/astro-ph/9711159
dc.identifierhttp://arxiv.org/abs/astro-ph/9711159
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11798
dc.subjectAstrophysics
dc.titleClustering of Absorbers
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