Cosmological Implications of X-ray Clusters of Galaxies

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dc.creatorSuto, Yasushi
dc.creatorKitayama, Tetsu
dc.creatorSasaki, Shin
dc.date1998-04-14
dc.date.accessioned2026-07-07T02:26:35Z
dc.date.available2026-07-07T02:26:35Z
dc.descriptionCosmological implications of clusters of galaxies are discussed with particular attention to their importance in probing the cosmological parameters. More specifically we compute the number counts of clusters of galaxies, Log $N$ -- Log $S$ relation, in X-ray and submm bands on the basis of the Press--Schechter theory. We pay particular attention to a set of theoretical models which well reproduce the {\it ROSAT} 0.5-2 keV band Log $N$ -- Log $S$, and explore possibilities to break the degeneracy among the viable cosmological models.
dc.description9 pages, to appear in the Proceedings of the 5th Taipei Astrophysics Workshop ``Cosmic Microwave Background and Large-Scale Structure of the Universe''
dc.identifierhttps://arxiv.org/abs/astro-ph/9804126
dc.identifierhttp://arxiv.org/abs/astro-ph/9804126
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12331
dc.subjectAstrophysics
dc.titleCosmological Implications of X-ray Clusters of Galaxies
dc.typetext

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