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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---2022-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">69</article-id>
      <article-id pub-id-type="doi">10.34898/aat.vol5.iss1.pp5-7</article-id>
      <article-categories>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Magnetism and Activity of the Sun - 2022 Conference proceedings</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="en">Dependence of starspot temperatures on the spectral type and luminosity of stars</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>Ilya</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>Kozhevnikova</surname>
              <given-names>Alla</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">Ural Federal University, Lenin av. 51, Ekaterinburg 620083</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2024-03-28">
        <day>28</day>
        <month>03</month>
        <year>2024</year>
      </pub-date>
      <volume>5</volume>
      <issue>1</issue>
      <fpage>5</fpage>
      <lpage>7</lpage>
      <history>
        <date date-type="received" iso-8601-date="2024-03-28">
          <day>28</day>
          <month>03</month>
          <year>2024</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>
					Copyright (c) 2026 Alekseev I., Kozhevnikova A.
				</copyright-statement>
        <copyright-year>
					2026
				</copyright-year>
        <copyright-holder>
					Ilya Alekseev, Alla Kozhevnikova
				</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/69"/>
      <abstract xml:lang="en">
        <p>  The paper considers the spottedness models for 54 stars with solar-type activity at different evolutionary stages (stars of different spectral types and luminosity classes). We note the dependence of starspot temperatures on the temperature of the undisturbed photosphere for stars at each stage of evolution (young post T Tau stars, dwarf stars on MS, and evolved giants). A weak dependence of starspot temperatures on the evolutionary stage of stars is shown. The general analytical expression for estimating starspot temperatures by the temperatures of undisturbed photospheres is obtained.  </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>stars</kwd>
        <kwd>starspots</kwd>
      </kwd-group>
      <funding-group>
        <funding-statement xml:lang="en">
                                                    The work of A. Kozhevnikova was supported by the Ministry of Science and Higher Education of the Russian Federation, project No. FEUZ-2020-0030
                                                </funding-statement>
      </funding-group>
      <counts>
        <page-count count="3"/>
      </counts>
    </article-meta>
  </front>
  <body/>
  <back>
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</article>
