<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
 <record>
  <leader>     naa a22        4500</leader>
  <controlfield tag="001">510789838</controlfield>
  <controlfield tag="003">CHVBK</controlfield>
  <controlfield tag="005">20180411083316.0</controlfield>
  <controlfield tag="007">cr unu---uuuuu</controlfield>
  <controlfield tag="008">180411e20130101xx      s     000 0 eng  </controlfield>
  <datafield tag="024" ind1="7" ind2="0">
   <subfield code="a">10.1134/S1063773713010039</subfield>
   <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="035" ind1=" " ind2=" ">
   <subfield code="a">(NATIONALLICENCE)springer-10.1134/S1063773713010039</subfield>
  </datafield>
  <datafield tag="245" ind1="0" ind2="0">
   <subfield code="a">HBHA 4705-03: A new cataclysmic variable</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[D. Yakin, V. Suleimanov, V. Vlasyuk, O. Spiridonova]</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
   <subfield code="a">Results of photometric and spectroscopic studies for the new eclipsing cataclysmic variable star HBHA 4705-03 with an orbital period of 0.1718 days are presented. Its spectrum exhibits hydrogen and helium emission lines. The Doppler maps constructed from hydrogen lines and the He II λ 4686 line show that the regions near the inner Lagrangian point are the main source of emission in these lines, while the maps constructed from He I lines suggest the presence of an accretion disk around the primary. The masses of the components (M WD = 0.54 ± 0.10M ⊙ andM RD = 0.45 ± 0.05 M ⊙) and the orbital inclination of the system (i = 71.8° ± 0.7°) have been determined from observational data using well-known relations for close binaries and cataclysmic variable stars.</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
   <subfield code="a">Pleiades Publishing, Ltd., 2013</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">binary stars</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">cataclysmic variables</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">HBHA 4705-03</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Yakin</subfield>
   <subfield code="D">D.</subfield>
   <subfield code="u">Kazan (Volga Region) Federal University, ul. Kremlevskaya 18, 420008, Kazan, Russia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Suleimanov</subfield>
   <subfield code="D">V.</subfield>
   <subfield code="u">Kazan (Volga Region) Federal University, ul. Kremlevskaya 18, 420008, Kazan, Russia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Vlasyuk</subfield>
   <subfield code="D">V.</subfield>
   <subfield code="u">Special Astrophysical Observatory, Russian Academy of Sciences, 357147, Nizhnii Arkhyz, Karachai-Cherkessian Republic, Russia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Spiridonova</subfield>
   <subfield code="D">O.</subfield>
   <subfield code="u">Special Astrophysical Observatory, Russian Academy of Sciences, 357147, Nizhnii Arkhyz, Karachai-Cherkessian Republic, Russia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="773" ind1="0" ind2=" ">
   <subfield code="t">Astronomy Letters</subfield>
   <subfield code="d">SP MAIK Nauka/Interperiodica</subfield>
   <subfield code="g">39/1(2013-01-01), 38-53</subfield>
   <subfield code="x">1063-7737</subfield>
   <subfield code="q">39:1&lt;38</subfield>
   <subfield code="1">2013</subfield>
   <subfield code="2">39</subfield>
   <subfield code="o">11443</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="0">
   <subfield code="u">https://doi.org/10.1134/S1063773713010039</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="908" ind1=" " ind2=" ">
   <subfield code="D">1</subfield>
   <subfield code="a">research-article</subfield>
   <subfield code="2">jats</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">856</subfield>
   <subfield code="E">40</subfield>
   <subfield code="u">https://doi.org/10.1134/S1063773713010039</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Yakin</subfield>
   <subfield code="D">D.</subfield>
   <subfield code="u">Kazan (Volga Region) Federal University, ul. Kremlevskaya 18, 420008, Kazan, Russia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Suleimanov</subfield>
   <subfield code="D">V.</subfield>
   <subfield code="u">Kazan (Volga Region) Federal University, ul. Kremlevskaya 18, 420008, Kazan, Russia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Vlasyuk</subfield>
   <subfield code="D">V.</subfield>
   <subfield code="u">Special Astrophysical Observatory, Russian Academy of Sciences, 357147, Nizhnii Arkhyz, Karachai-Cherkessian Republic, Russia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Spiridonova</subfield>
   <subfield code="D">O.</subfield>
   <subfield code="u">Special Astrophysical Observatory, Russian Academy of Sciences, 357147, Nizhnii Arkhyz, Karachai-Cherkessian Republic, Russia</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">773</subfield>
   <subfield code="E">0-</subfield>
   <subfield code="t">Astronomy Letters</subfield>
   <subfield code="d">SP MAIK Nauka/Interperiodica</subfield>
   <subfield code="g">39/1(2013-01-01), 38-53</subfield>
   <subfield code="x">1063-7737</subfield>
   <subfield code="q">39:1&lt;38</subfield>
   <subfield code="1">2013</subfield>
   <subfield code="2">39</subfield>
   <subfield code="o">11443</subfield>
  </datafield>
  <datafield tag="900" ind1=" " ind2="7">
   <subfield code="a">Metadata rights reserved</subfield>
   <subfield code="b">Springer special CC-BY-NC licence</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="898" ind1=" " ind2=" ">
   <subfield code="a">BK010053</subfield>
   <subfield code="b">XK010053</subfield>
   <subfield code="c">XK010000</subfield>
  </datafield>
  <datafield tag="949" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="F">NATIONALLICENCE</subfield>
   <subfield code="b">NL-springer</subfield>
  </datafield>
 </record>
</collection>
