{
  "id": "astro-ph/0106414",
  "version": "v1",
  "published": "2001-06-22T14:34:32.000Z",
  "updated": "2001-06-22T14:34:32.000Z",
  "title": "Observations of galaxies with future X-ray observatories",
  "authors": [
    "G. Fabbiano"
  ],
  "comment": "conference proceeding; New Century of X-Ray Astronomy Yokohama Symposia, Yokohama, Japan 6-8 March 2001 http://www.astro.isas.ac.jp/conference/newcentx/",
  "categories": [
    "astro-ph"
  ],
  "abstract": "Normal galaxies are faint and complex X-ray sources that provide very powerful probes for fundamental astrophysical questions. Examples include: the study of populations of X-ray emitting sources; the study of the entire spectrum of black-hole phenomena; and galaxy formation and evolution in interaction with the surrounding environment. While exciting, all these fields {\\bf require} Chandra sub-arcsecond resolution, and at least comparable spectral capabilities. They also require much large collecting areas. I argue that this is the direction we must plan for future X-ray observatories.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2001-06-22T14:34:32.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "x-ray observatories",
      "observations",
      "complex x-ray sources",
      "chandra sub-arcsecond resolution",
      "comparable spectral capabilities"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 576491
    }
  }
}