{
  "id": "2212.11434",
  "version": "v1",
  "published": "2022-12-22T00:53:48.000Z",
  "updated": "2022-12-22T00:53:48.000Z",
  "title": "A closer look at NGC 7314 nuclear region: a multiwavelength analysis of the Seyfert nucleus and its surroundings",
  "authors": [
    "Patrícia da Silva",
    "R. B. Menezes",
    "Y. Díaz",
    "A. Rodríguez-Ardila",
    "E. López-Navas",
    "P. Arévalo",
    "L. Hernández-García"
  ],
  "comment": "20 pages, 16 figures, 7 tables",
  "doi": "10.1093/mnras/stac3454",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "The central regions of galaxies harbouring active galactic nuclei (AGNs) can be quite complex, especially at high activity, presenting, besides variability, a variety of phenomena related, e.g. to ionization/excitation mechanisms. A detailed study is necessary in order to understand better those objects. For that reason, we performed a multiwavelength analysis of the nuclear region of the nearby Seyfert galaxy NGC 7314, using an optical data cube obtained with the Integral Field Unit from the Gemini Multi-Object Spectrograph, together with Hubble Space Telescope images, X-ray data from the XMM-Newton and the Nuclear Spectroscopic Telescope Array and radio data from Atacama Large Millimeter/Submillimeter Array. The goals were to study the nuclear and circumnuclear emission, the emission of the AGN and the gas kinematics. The optical spectrum shows the emission of a Seyfert nucleus, with broad components in the H$\\alpha$ and H$\\beta$ emission lines, characterising a type 1 AGN, with a spectrum rich in coronal emission lines. The spatial morphology of the [OIII]$\\lambda$5007 suggests the presence of an ionization cone, west of the nucleus, meanwhile the east cone seems to be obscured by dust. An extended [FeVII]$\\lambda$6087 emission was also detected, which could be possibly explained by a scenario involving photoionization+shocks mechanisms. X-rays analyses showed that there are variations in the flux; however, we did not detect any variations in the column density along the line of sight. Its variability may be a consequence of changes in the AGN accretion rate.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2022-12-22T00:53:48.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "nuclear region",
      "multiwavelength analysis",
      "seyfert nucleus",
      "closer look",
      "harbouring active galactic nuclei"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 20,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}