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 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Infocommunications and Radio Technologies</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Infocommunications and Radio Technologies</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>ИНФОКОММУНИКАЦИОННЫЕ И РАДИОЭЛЕКТРОННЫЕ ТЕХНОЛОГИИ</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="print">2587-9936</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">52842</article-id>
   <article-id pub-id-type="doi">10.15826/icrt.2018.01.4.26</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>АСТРОНОМИЯ (01.03.00)</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>ASTRONOMY (01.03.00)</subject>
    </subj-group>
    <subj-group>
     <subject>АСТРОНОМИЯ (01.03.00)</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">Detection of the kilomaser of water vapor in the Galaxy</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Обнаружение киломазера водяного пара в Галактике</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Volvach</surname>
       <given-names>L. </given-names>
      </name>
      <name xml:lang="en">
       <surname>Volvach</surname>
       <given-names>Larisa N </given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Вольвач</surname>
       <given-names>Александр Евгеньевич </given-names>
      </name>
      <name xml:lang="en">
       <surname>Volvach</surname>
       <given-names>Alexandr E </given-names>
      </name>
     </name-alternatives>
     <email>volvach@bk.ru</email>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Ларионов</surname>
       <given-names>Михаил Григорьевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Larionov</surname>
       <given-names>Michail Grigor'evich</given-names>
      </name>
     </name-alternatives>
     <bio xml:lang="ru">
      <p>доктор физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>doctor of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-3"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Crimean Astrophysical Observatory of the Russian Academy of Sciences</institution>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Crimean Astrophysical Observatory of the Russian Academy of Sciences</institution>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Крымская астрофизическая обсерватория</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Radio Astronomy and Geodynamics Department, Crimean Astrophysical Observatory</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <aff>
     <institution xml:lang="ru">Физический институт им. П. Н. Лебедева РАН</institution>
     <city>Москва</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">P. N. Lebedev Physical Institute, RAS</institution>
     <city>Moscow</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2018-12-25T21:43:07+03:00">
    <day>25</day>
    <month>12</month>
    <year>2018</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2018-12-25T21:43:07+03:00">
    <day>25</day>
    <month>12</month>
    <year>2018</year>
   </pub-date>
   <volume>1</volume>
   <issue>4</issue>
   <fpage>341</fpage>
   <lpage>349</lpage>
   <history>
    <date date-type="received" iso-8601-date="2018-12-20T20:22:29+03:00">
     <day>20</day>
     <month>12</month>
     <year>2018</year>
    </date>
   </history>
   <self-uri xlink:href="https://rusjbpc.ru/en/nauka/article/52842/view">https://rusjbpc.ru/en/nauka/article/52842/view</self-uri>
   <abstract xml:lang="ru">
    <p>Представлены результаты длительного мониторинга галактического мазерного источника IRAS 18316-0602 (G25.65+1.05) в линии водяного пара (переход 616-523, частота линии f=22.235 ГГц), выполненные на радиотелескопах РТ-22 (Симеиз). Более точное расстояние, полученное для IRAS 18316-0602 (12.5 кпк), и значение плотности потока излучения в максимуме вспышки (  ≈ 1.3 × 105Ян) делают этот источник самым мощным галактическим киломазером.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The results of long-term monitoring of the Galactic maser source IRAS 18316-0602 (G25.65+1.05) in the water-vapor line at frequency f = 22.235 GHz (616- 523 transitioin) carried out on the 22-m Simeiz radio telescopes are reported. The accurate distance estimate for IRAS 18316-0602 (12.5 kpc) and the flux density at the flare maximum ( ≈ 1.3 × 105 Jy) makes this the most powerful Galactic kilomaser known.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>радиотелескоп</kwd>
    <kwd>радиоизлучение</kwd>
    <kwd>вспышка</kwd>
    <kwd>мазер</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>radio telescope</kwd>
    <kwd>radio emission</kwd>
    <kwd>flash</kwd>
    <kwd>maser</kwd>
   </kwd-group>
  </article-meta>
 </front>
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  <p></p>
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