{
  "id": "1511.07638",
  "version": "v1",
  "published": "2015-11-24T10:43:06.000Z",
  "updated": "2015-11-24T10:43:06.000Z",
  "title": "Galactic Wind in NGC 4460: New Observations",
  "authors": [
    "D. V. Oparin",
    "A. V. Moiseev"
  ],
  "comment": "8 pages, 7 figures",
  "journal": "Astrophysical Bulletin, 2015, vol. 70, No.4, pp. 392-399",
  "doi": "10.1134/S1990341315040021",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "NGC4460 is an isolated lenticular galaxy, in which galactic wind has been earlier discovered as a gas outflow associated with circumnuclear regions of star formation. Using the results of observations in the Halpha line with the scanning Fabry-Perot interferometer on the SAO RAS 6-m telescope, we studied the kinematics of the ionized gas in this galaxy. The parameters of gas outflow from the plane of the galactic disk were refined within a simple geometric model. We show that it is impossible to characterize the wind by a fixed velocity value. Characteristic outflow velocities are within 30..80 km/s , and they are insufficient to make the swept-out matter ultimately leave the galaxy.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2015-11-24T10:43:06.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "85A05"
    ],
    "keywords": [
      "galactic wind",
      "observations",
      "gas outflow",
      "swept-out matter ultimately leave",
      "simple geometric model"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "journal": "Astrophysical Bulletin",
      "year": 2015,
      "month": "Oct",
      "volume": 70,
      "number": 4,
      "pages": 392
    },
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2015AstBu..70..392O"
    }
  }
}