A Study of Lyman-Alpha Quasar Absorbers in the Nearby Universe

dc.creatorImpey, C. D.
dc.creatorPetry, C. E.
dc.creatorFlint, K. P.
dc.date1999-05-28
dc.date.accessioned2026-07-07T10:51:31Z
dc.date.available2026-07-07T10:51:31Z
dc.descriptionSpectroscopy of ten quasars obtained with the Goddard High Resolution Spectrograph (GHRS) of the Hubble Space Telescope (HST) is presented. A clustering analysis reveals an excess of nearest neighbor line pairs on velocity scales of 250-750 km/s at a 95-98% confidence level. The hypothesis that the absorbers are randomly distributed in velocity space can be ruled out at the 99.8% confidence level. No two-point correlation power is detected (xi < 1 with 95% confidence). Lyman-alpha absorbers have correlation amplitudes on scales of 250-500 km/s at least 4-5 times smaller than the correlation amplitude of bright galaxies. A detailed comparison between absorbers in nearby galaxies is carried out on a limited subset of 11 Lyman- alpha absorbers where the galaxy sample in a large contiguous volume is complete to M_B = -16. Absorbers lie preferentially in regions of intermediate galaxy density but it is often not possible to uniquely assign a galaxy counterpart to an absorber. This sample provides no explicit support for the hypothesis that absorbers are preferentially associated with the halos of luminous galaxies. We have made a preliminary comparison of the absorption line properties and environments with the results of hydrodynamic simulations. The results suggest that the Lyman-alpha absorbers represent diffuse or shocked gas in the IGM that traces the cosmic web of large scale structure. (abridged)
dc.description36 pages of text, 15 figures, 4 tables, 36 files
dc.identifierhttps://arxiv.org/abs/astro-ph/9905381
dc.identifierhttp://arxiv.org/abs/astro-ph/9905381
dc.identifierAstrophys.J.524:536,1999
dc.identifierdoi:10.1086/307845
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184842
dc.subjectAstrophysics
dc.titleA Study of Lyman-Alpha Quasar Absorbers in the Nearby Universe
dc.typetext

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