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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="материалы-конференции-&quot;магнетизм-и-активность-солнца-и-звезд----2021&quot;" xml:lang="ru">
  <front>
    <journal-meta>
      <journal-id journal-id-type="ojs">izvcrao</journal-id>
      <journal-id journal-id-type="publisher-id" xml:lang="ru">
                       Изв. Крымск. Астрофиз. Обсерв.
                </journal-id>
      <journal-id journal-id-type="publisher-id" xml:lang="en">
                        Izv. Krymsk. Astrofiz. Observ.
                    </journal-id>
      <journal-title-group>
        <journal-title xml:lang="ru">
                    Известия Крымской астрофизической обсерватории
                </journal-title>
        <trans-title-group xml:lang="en">
          <trans-title>Izvestiya Krymskoi Astrofizicheskoi Observatorii</trans-title>
        </trans-title-group>
      </journal-title-group>
      <issn pub-type="ppub">0367-8466</issn>
      <issn pub-type="epub">3034-4107</issn>
      <publisher>
        <publisher-name>Киселев Н.Н., пос. Московский, Москва, РФ</publisher-name>
        <publisher-loc>RU</publisher-loc>
      </publisher>
      <self-uri xlink:href="https://jncrao.ru/index.php/izvcrao"/>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="publisher-id">1084</article-id>
      <article-id pub-id-type="doi">10.34898/izcrao-vol118-iss3-pp5-18</article-id>
      <article-categories>
        <subj-group xml:lang="ru" subj-group-type="heading">
          <subject>Материалы конференции "Магнетизм и активность Солнца и звезд  - 2021"</subject>
        </subj-group>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Magnetism and activity of the Sun and stars  – 2021 Conference proceedings</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="ru">Идентификация объектов оптического диапазона в областях жесткого излучения вблизи красных карликовых звезд</article-title>
        <trans-title-group xml:lang="en">
          <trans-title>Identification of objects in the optical range in the areas of hard radiation near red dwarf stars</trans-title>
        </trans-title-group>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="ru" specific-use="primary">
              <surname>Шляпников</surname>
              <given-names>Алексей</given-names>
            </name>
            <name name-style="western" xml:lang="en" specific-use="">
              <surname>Shlyapnikov</surname>
              <given-names>Aleksei</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="ru">ФГБУН "Крымская астрофизическая обсерватория РАН",  Научный, Крым, 298409</institution>
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory, Nauchny, 298409</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2022-12-20">
        <day>20</day>
        <month>12</month>
        <year>2022</year>
      </pub-date>
      <volume>118</volume>
      <issue>3</issue>
      <fpage>5</fpage>
      <lpage>18</lpage>
      <history>
        <date date-type="received" iso-8601-date="2021-11-05">
          <day>05</day>
          <month>11</month>
          <year>2021</year>
        </date>
      </history>
      <permissions>
        <copyright-statement xml:lang="ru">Copyright (c) 2022 Шляпников А.</copyright-statement>
        <copyright-statement xml:lang="en">Copyright (c) 2022 Shlyapnikov A.</copyright-statement>
        <copyright-year>
					2022
				</copyright-year>
        <copyright-holder xml:lang="ru">Шляпников А.</copyright-holder>
        <copyright-holder xml:lang="en">Shlyapnikov A.</copyright-holder>
        <license license-type="open-access" xlink:href="http://creativecommons.org/licenses/by/4.0" xml:lang="ru">
          <license-p> Метаданные этой статьи доступны по лицензии  Creative Commons «Attribution» («Атрибуция») 4.0 Всемирная.  
 Авторское право и право на публикацию текстов, представленных в журнале  "Известия Крымской астрофизической обсерватории", сохраняются за авторами, при этом право первой публикации предоставляется журналу. Тексты могут свободно использоваться при условии правильного цитирования с указанием авторства в соответствии с лицензией  Creative Commons «Attribution» («Атрибуция») 4.0 Всемирная.  
     </license-p>
        </license>
        <license license-type="open-access" xlink:href="http://creativecommons.org/licenses/by/4.0" xml:lang="en">
          <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 Izvestiya Krymskoi Astrofizicheskoi Observatorii 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://jncrao.ru/index.php/izvcrao/article/view/1084"/>
      <abstract xml:lang="ru">
        <p>  Проведен анализ областей локализации источников ТэВ гамма-излучения в рентгеновском и оптическом диапазонах спектра. Указаны угловые расстояния от положения максимумов в распределении высокоэнергетических потоков до вероятных кандидатов на идентификацию с красными карликами. Также рассмотрены возможные отождествления более слабых ТэВ-источников и других объектов поля.  </p>
      </abstract>
      <abstract xml:lang="en">
        <p>  The analysis of the localization regions of TeV gamma-ray sources in the X-ray and optical spectral ranges is carried out. The angle distances from the position of the maxima in the distribution of high-energy fluxes to the probable candidates for identification with red dwarfs are indicated. Possible identifications of fainter TeV sources and other field objects are also considered.  </p>
      </abstract>
      <kwd-group xml:lang="ru">
        <kwd>звезды - переменные и пекулярные</kwd>
        <kwd>рентгеновские и гамма-источники</kwd>
      </kwd-group>
      <funding-group>
        <funding-statement xml:lang="ru">
                                                    РФФИ № 19-02-00191 и № 19-29-11027
                                                </funding-statement>
      </funding-group>
      <counts>
        <page-count count="14"/>
      </counts>
    </article-meta>
  </front>
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