New Results on the Coma cluster: Revealing the Primary Component

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dc.creatorDurret, F.
dc.creatorBiviano, A.
dc.creatorGerbal, D.
dc.creatorFevre, O. Le
dc.creatorLobo, C.
dc.creatorMazure, A.
dc.creatorSlezak, E.
dc.date1995-08-31
dc.date.accessioned2026-07-07T02:20:06Z
dc.date.available2026-07-07T02:20:06Z
dc.descriptionRecent observations of the Coma cluster of galaxies in its central region have provided approximately 250 new redshifts - allowing a good membership criterion to be established for brighter galaxies - and magnitudes for 8000 objects in the same region derived from photometric data complete up to V$_{26.5}$=22.5. A thorough structural study of the galaxy distribution of the cluster galaxies, jointly with an X-ray wavelet analysis, and with a kinematical analysis of the velocity distribution allows us to uncover a primary body of the cluster, with evidence for a velocity gradient.
dc.descriptionPostScript, 8 pages with figures, to appear in the proceedings of the workshop "Observational Cosmology: from Galaxies to Galaxy Systems", Sesto-Italy, 4-7 July 1995, in a devoted issue of Astrophysical Letters and Communications
dc.identifierhttps://arxiv.org/abs/astro-ph/9508153
dc.identifierhttp://arxiv.org/abs/astro-ph/9508153
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10108
dc.subjectAstrophysics
dc.titleNew Results on the Coma cluster: Revealing the Primary Component
dc.typetext

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