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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="magnetism-and-activity-of-the-sun-and-stars--–-2021-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">40</article-id>
      <article-id pub-id-type="doi">10.34898/aat.vol3.iss2.pp27-29</article-id>
      <article-categories>
        <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="en">On the temperature of starspots</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Alekseev</surname>
              <given-names>I.Yu. </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>Gershberg</surname>
              <given-names> R.E. </given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-2"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory, Nauchny 298409</institution>
      </aff>
      <aff id="aff-2">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory, Nauchny, 298409</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2022-06-15">
        <day>15</day>
        <month>06</month>
        <year>2022</year>
      </pub-date>
      <volume>3</volume>
      <issue>2</issue>
      <fpage>27</fpage>
      <lpage>29</lpage>
      <history>
        <date date-type="received" iso-8601-date="2022-06-15">
          <day>15</day>
          <month>06</month>
          <year>2022</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>
					Copyright (c)  Alekseev I., Gershberg R.
				</copyright-statement>
        <copyright-year>
					
				</copyright-year>
        <copyright-holder>
					Alekseev I., Gershberg  .
				</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/40"/>
      <abstract xml:lang="en">
        <p>  A number of models of the zonal spottedness of stars with solar-type activity show a certain correlation between starspot temperatures and temperatures of quiet photospheres.   </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>Stars: starspots</kwd>
      </kwd-group>
      <counts>
        <page-count count="3"/>
      </counts>
    </article-meta>
  </front>
  <body/>
  <back>
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</article>
