{
  "id": "1611.07872",
  "version": "v1",
  "published": "2016-11-23T16:39:33.000Z",
  "updated": "2016-11-23T16:39:33.000Z",
  "title": "Correlations between Supermassive Black Holes and their Hosts in Active Galaxies",
  "authors": [
    "Gerold Busch"
  ],
  "comment": "8 pages, 2 figures; to appear in the Proceedings of the 25th Annual Conference of Doctoral Students (WDS 2016), Prague",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "In the last decades several correlations between the mass of the central supermassive black hole (BH) and properties of the host galaxy - such as bulge luminosity and mass, central stellar velocity dispersion, S\\'ersic index, spiral pitch angle etc. - have been found and point at a coevolution scenario of BH and host galaxy. In this article, I review some of these relations for inactive galaxies and discuss the findings for galaxies that host an active galactic nucleus/quasar. I present the results of our group that finds that active galaxies at $z\\lesssim 0.1$ do not follow the BH mass - bulge luminosity relation. Furthermore, I show near-infrared integral-field spectroscopic data that suggest that young stellar populations cause the bulge overluminosity and indicate that the host galaxy growth started first. Finally, I discuss implications for the BH-host coevolution.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-11-23T16:39:33.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "active galaxies",
      "correlations",
      "central stellar velocity dispersion",
      "host galaxy growth started first",
      "bulge luminosity relation"
    ],
    "tags": [
      "conference paper",
      "dissertation"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}