A Comparison of the EUV and X-Ray Emission Profiles in Six Clusters of Galaxies

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dc.creatorDurret, F.
dc.creatorSantos, S. Dos
dc.creatorLieu, R.
dc.date2001-05-29
dc.date.accessioned2026-07-07T01:58:43Z
dc.date.available2026-07-07T01:58:43Z
dc.descriptionWe have performed the wavelet analysis and image reconstructions for six clusters of galaxies observed both at extreme ultraviolet and X-ray energies. The comparison of the profiles of the EUV and X-ray reconstructed images shows that they differ at a very large confidence level in five of the six clusters, and are similar only for the Coma cluster, which is by far the hottest one in the sample.
dc.description14 pages, 9 PostScript figures, 2 JPEG figures. To appear in Proceedings of XXI Moriond Conference: "Galaxy Clusters and the High Redshift Universe Observed in X-rays", edited by D. Neumann, F. Durret, & J. Tran Thanh Van
dc.identifierhttps://arxiv.org/abs/astro-ph/0105498
dc.identifierhttp://arxiv.org/abs/astro-ph/0105498
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2824
dc.subjectAstrophysics
dc.titleA Comparison of the EUV and X-Ray Emission Profiles in Six Clusters of Galaxies
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