The power spectrum of the Lyman--$α$ clouds

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dc.creatorAmendola, L.
dc.creatorSavaglio, S.
dc.date1997-09-16
dc.date.accessioned2026-07-07T02:24:15Z
dc.date.available2026-07-07T02:24:15Z
dc.descriptionWe estimate the 1--D power spectrum and the integral density of neighbors in 14 QSO lines of sight. We discuss their variation with respect to redshift and column density and compare the results with standard CDM models.
dc.description2 pages, 1 ps figure. To appear in the Proceedings of the 13th IAP Colloquium on "Structure and Evolution of the IGM from QSO Absorption Lines", ed. P. Petitjean, S. Charlot, Paris July 1-5
dc.identifierhttps://arxiv.org/abs/astro-ph/9709155
dc.identifierhttp://arxiv.org/abs/astro-ph/9709155
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11550
dc.subjectAstrophysics
dc.titleThe power spectrum of the Lyman--$α$ clouds
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