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  <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">50</article-id>
      <article-id pub-id-type="doi">10.34898/aat.vol4.iss1.pp8-11</article-id>
      <article-categories>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Сonference proceedings</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="en">The optical and infrared study of an active star-formation region in the southern part of Mon R2</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Movsessian</surname>
              <given-names>Tigran</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-1"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Magakian</surname>
              <given-names>Tigran</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-2"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Bally</surname>
              <given-names>John</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-3"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Moiseev</surname>
              <given-names>Aleksei</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-4"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Andreasyan</surname>
              <given-names>Hasmik</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-5"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">Byurakan Observatory of the National Academy of Sciences of Armenia, Byurakan, Aragatsotn prov., 0213, Armenia</institution>
      </aff>
      <aff id="aff-2">
        <institution content-type="orgname" xml:lang="en">Byurakan Observatory of the National Academy of Sciences of Armenia, Byurakan, Aragatsotn prov., 0213, Armenia</institution>
      </aff>
      <aff id="aff-3">
        <institution content-type="orgname" xml:lang="en">Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO, USA</institution>
      </aff>
      <aff id="aff-4">
        <institution content-type="orgname" xml:lang="en">Special Astrophysical Observatory, Nizhniy Arkhyz, Karachaevo-Cherkesia, 369167 Russia</institution>
      </aff>
      <aff id="aff-5">
        <institution content-type="orgname" xml:lang="en">Byurakan Observatory of the National Academy of Sciences of Armenia, Byurakan, Aragatsotn prov., 0213, Armenia</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2023-09-28">
        <day>28</day>
        <month>09</month>
        <year>2023</year>
      </pub-date>
      <volume>4</volume>
      <issue>1</issue>
      <fpage>8</fpage>
      <lpage>11</lpage>
      <history>
        <date date-type="received" iso-8601-date="2022-10-24">
          <day>24</day>
          <month>10</month>
          <year>2022</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>
					Copyright (c) 2026 Movsessian T., Magakian T., Bally J., Moiseev A., Andreasyan H.
				</copyright-statement>
        <copyright-year>
					2026
				</copyright-year>
        <copyright-holder>
					Tigran Movsessian, Tigran Magakian, John Bally, Aleksei Moiseev, Hasmik Andreasyan
				</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/50"/>
      <abstract xml:lang="en">
        <p> This is a shortened version of the presentation at the conference “Non-Stationary Processes in the Protoplanetary Disks and Their Observational Manifestations” held at the Crimean Astrophysical Observatory. 
 We present narrow-band images of the southern part of the Mon R2 association obtained in the course of the BNBIS survey with the 1-m Schmidt telescope of the Byurakan Observatory. The main task of this survey is search and study of new Herbig-Haro (HH) objects and collimated outflows using the narrow-band H α  and [S ii] images of certain fields in dark clouds of the Galaxy since the presence of HH objects is one of the main indicators of active star-formation processes. 
 Several new HH objects and outflow systems were discovered, including the helical chain of HH objects near IRAS 06068-0643 (V963 Mon) and the curved outflow system associated with the 2MASS 06084223-0657385 source, which probably represents the irradiated giant outflow. Also, two molecular hydrogen outflows associated with deeply embedded IR sources near the 2MASS 06084223-0657385 region were revealed. </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>YSO’s</kwd>
        <kwd>Herbig-Haro objecys</kwd>
        <kwd>outflows</kwd>
      </kwd-group>
      <funding-group>
        <funding-statement xml:lang="en">
                                                    This work was partly supported by RA State Committee of Science, in the frames of the research project 21T-1C031
                                                </funding-statement>
      </funding-group>
      <counts>
        <page-count count="4"/>
      </counts>
    </article-meta>
  </front>
  <body/>
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</article>
