{
  "id": "astro-ph/9508153",
  "version": "v1",
  "published": "1995-08-31T13:53:15.000Z",
  "updated": "1995-08-31T13:53:15.000Z",
  "title": "New Results on the Coma cluster: Revealing the Primary Component",
  "authors": [
    "F. Durret",
    "A. Biviano",
    "D. Gerbal",
    "O. Le Fevre",
    "C. Lobo",
    "A. Mazure",
    "E. Slezak"
  ],
  "comment": "PostScript, 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",
  "categories": [
    "astro-ph"
  ],
  "abstract": "Recent 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.",
  "revisions": [
    {
      "version": "v1",
      "updated": "1995-08-31T13:53:15.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "coma cluster",
      "primary component",
      "thorough structural study",
      "x-ray wavelet analysis",
      "photometric data complete"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 412848
    }
  }
}