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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" article-type="crimean-2021-agn-conference-proceedings" xml:lang="en">
  <front>
    <journal-meta>
      <journal-id journal-id-type="ojs">aat</journal-id>
      <journal-id journal-id-type="publisher-id" xml:lang="en">
                       Acta Astrophys. Tau.
                </journal-id>
      <journal-title-group>
        <journal-title xml:lang="en">
                    Acta Astrophysica Taurica
                </journal-title>
      </journal-title-group>
      <issn pub-type="epub">2712-925X</issn>
      <publisher>
        <publisher-name>Kiselev Nikolai Nikolaevich,  Mosсow, settlement Moskovskii, Tat'yanin Park Str., 12, Moscow, Russia.</publisher-name>
        <publisher-loc>RU</publisher-loc>
      </publisher>
      <self-uri xlink:href="https://astrophysicatauricum.org/index.php/aat"/>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="publisher-id">32</article-id>
      <article-id pub-id-type="doi">10.31059/aat.vol3.iss1.pp23-26</article-id>
      <article-categories>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Crimean-2021 AGN Conference proceedings</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="en">Misalignments in NGC 1068</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Vermot</surname>
              <given-names>Pierre</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-1"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">Astronomical Institute, Academy of Sciences, Boční II 1401, Prague, Czech Republic; LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, 5 place Jules Janssen, 92195 Meudon, France</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2022-03-14">
        <day>14</day>
        <month>03</month>
        <year>2022</year>
      </pub-date>
      <volume>3</volume>
      <issue>1</issue>
      <fpage>23</fpage>
      <lpage>26</lpage>
      <history>
        <date date-type="received" iso-8601-date="2021-12-01">
          <day>01</day>
          <month>12</month>
          <year>2021</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>
					Copyright (c)  Vermot P.
				</copyright-statement>
        <copyright-year>
					
				</copyright-year>
        <copyright-holder>
					Vermot P.
				</copyright-holder>
        <license xlink:href="http://creativecommons.org/licenses/by/4.0">
          <license-p> The metadata for this submission is licensed under a  Creative Commons Attribution 4.0 International License.  
 Copyright and publishing rights for texts published in  Acta Astrophysica Taurica  is retained by the authors, with first publication rights granted to the journal.Texts are free to use with proper attribution and link to the licensing  (Creative Commons Attribution 4.0 International).  
     </license-p>
        </license>
      </permissions>
      <self-uri xlink:href="https://astrophysicatauricum.org/index.php/aat/article/view/32"/>
      <abstract xml:lang="en">
        <p> NGC 1068 is a nearby Active Galactic Nuclei (AGN) of type 2, meaning that its accretion disk is hidden behind a large amount of foreground extinction. Observations at several wavelengths have revealed various disk-like structures around the nucleus, all possibly part of the putative torus responsible for the obscuration of the AGN. I present results based on a GRAVITY/VLTI interferometric observation in the near-infrared, which provides very high angular resolution and gives insights into the geometry of the innermost region of this torus. The 3D orientation of the structure is surprising in several aspects, as it is misaligned with other disks present around the nucleus, and leaves a clear line of sight toward the central source. </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>NGC 1068</kwd>
        <kwd>Active Galactic Nuclei</kwd>
        <kwd>GRAVITY</kwd>
        <kwd>dust</kwd>
      </kwd-group>
      <funding-group>
        <funding-statement xml:lang="en">
                                                    Czech Science Foundation Grant 19-15480S
                                                </funding-statement>
      </funding-group>
      <counts>
        <page-count count="4"/>
      </counts>
    </article-meta>
  </front>
  <body/>
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</article>
