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 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Journal of Natural Sciences Research</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Journal of Natural Sciences Research</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Журнал естественнонаучных исследований</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="print">2500-0489</issn>
   <issn publication-format="online">2500-0489</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">91697</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>Астрофизика</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>Astrophysics</subject>
    </subj-group>
    <subj-group>
     <subject>Астрофизика</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">The Mechanism of Formation of &quot;Odd Radio Circles&quot;</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Механизм формирования «странных радио-кругов»</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Поройков</surname>
       <given-names>С. Ю.</given-names>
      </name>
      <name xml:lang="en">
       <surname>Poroikov</surname>
       <given-names>Sergey Yu.</given-names>
      </name>
     </name-alternatives>
     <email>sporoykov@mail.ru</email>
     <bio xml:lang="ru">
      <p>кандидат физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>candidate of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Московский государственный университет имени М.В.Ломоносова</institution>
    </aff>
    <aff>
     <institution xml:lang="en">Lomonosov Moscow State University</institution>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2024-12-08T23:20:50+03:00">
    <day>08</day>
    <month>12</month>
    <year>2024</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2024-12-08T23:20:50+03:00">
    <day>08</day>
    <month>12</month>
    <year>2024</year>
   </pub-date>
   <volume>9</volume>
   <issue>4</issue>
   <fpage>82</fpage>
   <lpage>99</lpage>
   <history>
    <date date-type="received" iso-8601-date="2024-10-09T00:00:00+03:00">
     <day>09</day>
     <month>10</month>
     <year>2024</year>
    </date>
    <date date-type="accepted" iso-8601-date="2024-11-01T00:00:00+03:00">
     <day>01</day>
     <month>11</month>
     <year>2024</year>
    </date>
   </history>
   <self-uri xlink:href="https://naukaru.ru/en/nauka/article/91697/view">https://naukaru.ru/en/nauka/article/91697/view</self-uri>
   <abstract xml:lang="ru">
    <p>Обнаружены «странные радио-круги» диаметром до 300 кпк, содержащие десятки сфериче-ских сгустков диаметром ~15 кпк. Теплый газ в радио-кругах излучает в УФ линиях ряда ионов (О, Mg, Ne) с температурой ~104 К, уширенных динамикой газа (~200 км/с), обуслов-ленной ударной волной. Излучение в оптическом и ближнем ИК диапазоне связано со звездным континуумом. Радио-круг могут образовать ударные волны сверхновых, усилен-ные звездным ветром голубых звезд в звездном потоке возрастом ≥109 лет, содержащем ≥3∙108 звезд, образованном галактикой массой ~1010 М○. Звездообразование в звездном по-токе может инициировать газ, нагребенный ударной волной (оттекающий в ее хвост), обра-зуемой вокруг газовой короны галактики – спутника, движущейся в межгалактическом газе.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>&quot;Odd radio circles&quot; up to 300 kpc in diameter, containing dozens of spherical clumps ~15 kpc in di-ameter were detected. Warm gas in the radio circles emits in the UV lines of a number of ions (O, Mg, Ne) with a temperature of ~104 K, broadened by the gas dynamics (~200 km/s) caused by the shock wave. Emission in the optical and near-IR ranges is associated with the stellar continuum. The radio circle may be formed by supernova shock waves amplified by the stellar wind of blue stars in a stellar stream ≥109 years old, containing ≥3∙108 stars, formed by a galaxy with a mass of ~1010 M○. Star formation in a stellar stream can be initiated by gas raked by a shock wave (flowing into its tail) formed around the gas corona of a satellite galaxy moving in intergalactic gas.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>странные радио-круги</kwd>
    <kwd>звездные потоки</kwd>
    <kwd>сверхновые</kwd>
    <kwd>звездный ветер</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>odd radio circles</kwd>
    <kwd>star streams</kwd>
    <kwd>supernovae</kwd>
    <kwd>stellar wind</kwd>
   </kwd-group>
  </article-meta>
 </front>
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  <p></p>
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