arXiv:astro-ph/9711159AbstractReferencesReviewsResources
Clustering of Absorbers
S. Cristiani, S. D'Odorico, V. D'Odorico, A. Fontana, E. Giallongo, L. Moscardini, S. Savaglio
Published 1997-11-14Version 1
The observed clustering of Lyman-$\alpha$ lines is reviewed and compared with the clustering of CIV systems. We argue that a continuity of properties exists between Lyman-$\alpha$ 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.
Comments: 8 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
Categories: astro-ph
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