X-ray Surveys of Low-redshift Clusters

dc.creatorEdge, Alastair C.
dc.date2003-07-08
dc.date.accessioned2026-07-07T02:08:56Z
dc.date.available2026-07-07T02:08:56Z
dc.descriptionThe selection of clusters of galaxies through their X-ray emission has proved to be an extremely powerful technique over the past four decades. The growth of X-ray astronomy has provided the community with a steadily more detailed view of the intracluster medium in clusters. In this review I will assess how far X-ray surveys of clusters have progressed and how far they still have to travel.
dc.description14 pages, 2 figures Carnegie Observatories Astrophysics Series, Vol. 3: Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution, ed. J. S. Mulchaey, A. Dressler, and A. Oemler (Cambridge: Cambridge Univ. Press)
dc.identifierhttps://arxiv.org/abs/astro-ph/0307150
dc.identifierhttp://arxiv.org/abs/astro-ph/0307150
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6256
dc.subjectAstrophysics
dc.titleX-ray Surveys of Low-redshift Clusters
dc.typetext

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