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  <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">230</article-id>
      <article-categories>
        <subj-group xml:lang="ru" subj-group-type="heading">
          <subject>Материалы конференции</subject>
        </subj-group>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Сonference proceedings</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="ru">Radio Relics in Clusters of Galaxies: A unique case of Abell 548b</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="">
              <surname>Tsarevsky</surname>
              <given-names>G.</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="">
              <surname>Feretti</surname>
              <given-names>L.</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="">
              <surname>Andernach</surname>
              <given-names>H.</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="">
              <surname>Bacchi</surname>
              <given-names>M.</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="">
              <surname>Slee</surname>
              <given-names>O.B.</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-5"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="">
              <surname>Giovannini</surname>
              <given-names>G.</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-6"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="">
              <surname>Govoni</surname>
              <given-names>F.</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-7"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="ru">Astro Space Center, Academy of Science, 84/32 Profsoyuznaya St., Moscow, 117910 Russia; Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, NSW 1710, Australia</institution>
      </aff>
      <aff id="aff-2">
        <institution content-type="orgname" xml:lang="ru">INAF Istituto di Radioastronomia, via P. Gobetti 101, I–40129 Bologna, Italy</institution>
      </aff>
      <aff id="aff-3">
        <institution content-type="orgname" xml:lang="ru">Departamento de Astronom´ıa, Universidad de Guanajuato, AP 144, Guanajuato CP 36000, Mexico</institution>
      </aff>
      <aff id="aff-4">
        <institution content-type="orgname" xml:lang="ru">INAF Istituto di Radioastronomia, via P. Gobetti 101, I–40129 Bologna, Italy</institution>
      </aff>
      <aff id="aff-5">
        <institution content-type="orgname" xml:lang="ru">Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, NSW 1710, Australia</institution>
      </aff>
      <aff id="aff-6">
        <institution content-type="orgname" xml:lang="ru">Dipartimento di Astronomia, Univ. Bologna, via Ranzani 1, I-40127 Bologna, Italy; INAF Istituto di Radioastronomia, via P. Gobetti 101, I–40129 Bologna, Italy</institution>
      </aff>
      <aff id="aff-7">
        <institution content-type="orgname" xml:lang="ru">INAF Istituto di Radioastronomia, via P. Gobetti 101, I–40129 Bologna, Italy; INAF Osservatorio Astronomico di Cagliari, Loc. Poggio dei Pini, Strada 54, 09012 Capoterra, Italy</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2007-07-01">
        <day>01</day>
        <month>07</month>
        <year>2007</year>
      </pub-date>
      <volume>103</volume>
      <issue>3</issue>
      <fpage>37</fpage>
      <lpage>42</lpage>
      <history>
        <date date-type="received" iso-8601-date="2017-09-25">
          <day>25</day>
          <month>09</month>
          <year>2017</year>
        </date>
      </history>
      <permissions>
        <copyright-statement xml:lang="ru">Copyright (c) 2007 , , , , , , </copyright-statement>
        <copyright-statement xml:lang="en">Copyright (c) 2007 Tsarevsky G., Feretti L., Andernach H., Bacchi M., Slee O., Giovannini G., Govoni F.</copyright-statement>
        <copyright-year>
					2007
				</copyright-year>
        <copyright-holder xml:lang="ru">, , , , , , </copyright-holder>
        <copyright-holder xml:lang="en">Tsarevsky G., Feretti L., Andernach H., Bacchi M., Slee O., Giovannini G., Govoni F.</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/230"/>
      <abstract xml:lang="ru">
        <p> Currently about 30 clusters of galaxies are known to have diffuse radio sources (so-called relics), but detailed studies are available for only a few. A548b, a rich and X-ray bright cluster of galaxies, is one of only three clusters (together with A3376 and A3667) known to contain two relics. From our investigation based on multi-wavelength ATCA and VLA observations, we found that both relics (A and B), located on the same side of the cluster’s center, show similar flux, extent, shape, high level of polarization and very steep spectral index. We conclude that these sources are likely related to the merger activity in the cluster. We have also possibly detected a centrally projected third relic (C). If confirmed, it would make A548b a unique triple-relic cluster. </p>
      </abstract>
      <counts>
        <page-count count="6"/>
      </counts>
    </article-meta>
  </front>
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