Shape and geometry of galaxy clusters and the SZ effect

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dc.creatorGrenacher, L.
dc.creatorPiffaretti, R.
dc.creatorPuy, D.
dc.creatorJetzer, Ph.
dc.creatorSignore, M.
dc.date2000-10-25
dc.date.accessioned2026-07-07T01:56:13Z
dc.date.available2026-07-07T01:56:13Z
dc.descriptionWe discuss the influence of the finite extension and the geometry of clusters of galaxies, as well as of the polytropic temperature profile, on the determination of the Hubble constant.
dc.description9 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0010512
dc.identifierhttp://arxiv.org/abs/astro-ph/0010512
dc.identifierTalk given at the workshop SZ in Toulouse, Toulouse (France), May 29-30, 2000
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1917
dc.subjectAstrophysics
dc.titleShape and geometry of galaxy clusters and the SZ effect
dc.typetext

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