<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
<record>
  <controlfield tag="001">124452</controlfield>
  <controlfield tag="005">20241125101150.0</controlfield>
  <datafield tag="024" ind1="7" ind2=" ">
    <subfield code="2">doi</subfield>
    <subfield code="a">10.1007/s10569-022-10118-z</subfield>
  </datafield>
  <datafield tag="024" ind1="8" ind2=" ">
    <subfield code="2">sideral</subfield>
    <subfield code="a">132851</subfield>
  </datafield>
  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ART-2023-132851</subfield>
  </datafield>
  <datafield tag="041" ind1=" " ind2=" ">
    <subfield code="a">eng</subfield>
  </datafield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Abad, A.</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
    <subfield code="0">(orcid)0000-0002-5692-5876</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Evolution of the characteristic curves in the restricted three-body problem in terms of the mass parameter</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2023</subfield>
  </datafield>
  <datafield tag="506" ind1="0" ind2=" ">
    <subfield code="a">Access copy available to the general public</subfield>
    <subfield code="f">Unrestricted</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
    <subfield code="a">In this work, we study the evolution of the families of simple symmetric periodic orbits in the restricted three-body problem whatever the value of the mass parameter μ. To classify these characteristic curves, we introduce a topological characterization of both orbits and families. Starting from the work of Strömgren for the Copenhagen case, we analyze the evolution of these families, when the mass parameter μ varies in (0, 1/2], focusing on their topological characterization, the existence of asymptotic points and the appearance of certain types of orbits such as horseshoe orbits. Lastly, we consider two samples, the Earth–Moon and Sun–Jupiter systems and classify the different types of orbits for these systems.</subfield>
  </datafield>
  <datafield tag="536" ind1=" " ind2=" ">
    <subfield code="9">info:eu-repo/grantAgreement/ES/DGA-FSE/E24-20R</subfield>
    <subfield code="9">info:eu-repo/grantAgreement/ES/MICINN/PID2020-117066GB-I00</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
    <subfield code="9">info:eu-repo/semantics/openAccess</subfield>
    <subfield code="a">by</subfield>
    <subfield code="u">http://creativecommons.org/licenses/by/3.0/es/</subfield>
  </datafield>
  <datafield tag="590" ind1=" " ind2=" ">
    <subfield code="a">1.6</subfield>
    <subfield code="b">2023</subfield>
  </datafield>
  <datafield tag="591" ind1=" " ind2=" ">
    <subfield code="a">MATHEMATICS, INTERDISCIPLINARY APPLICATIONS</subfield>
    <subfield code="b">70 / 135 = 0.519</subfield>
    <subfield code="c">2023</subfield>
    <subfield code="d">Q3</subfield>
    <subfield code="e">T2</subfield>
  </datafield>
  <datafield tag="591" ind1=" " ind2=" ">
    <subfield code="a">ASTRONOMY &amp; ASTROPHYSICS</subfield>
    <subfield code="b">51 / 84 = 0.607</subfield>
    <subfield code="c">2023</subfield>
    <subfield code="d">Q3</subfield>
    <subfield code="e">T2</subfield>
  </datafield>
  <datafield tag="592" ind1=" " ind2=" ">
    <subfield code="a">0.521</subfield>
    <subfield code="b">2023</subfield>
  </datafield>
  <datafield tag="593" ind1=" " ind2=" ">
    <subfield code="a">Applied Mathematics</subfield>
    <subfield code="c">2023</subfield>
    <subfield code="d">Q2</subfield>
  </datafield>
  <datafield tag="593" ind1=" " ind2=" ">
    <subfield code="a">Astronomy and Astrophysics</subfield>
    <subfield code="c">2023</subfield>
    <subfield code="d">Q2</subfield>
  </datafield>
  <datafield tag="593" ind1=" " ind2=" ">
    <subfield code="a">Computational Mathematics</subfield>
    <subfield code="c">2023</subfield>
    <subfield code="d">Q2</subfield>
  </datafield>
  <datafield tag="593" ind1=" " ind2=" ">
    <subfield code="a">Mathematical Physics</subfield>
    <subfield code="c">2023</subfield>
    <subfield code="d">Q2</subfield>
  </datafield>
  <datafield tag="593" ind1=" " ind2=" ">
    <subfield code="a">Modeling and Simulation</subfield>
    <subfield code="c">2023</subfield>
    <subfield code="d">Q2</subfield>
  </datafield>
  <datafield tag="593" ind1=" " ind2=" ">
    <subfield code="a">Space and Planetary Science</subfield>
    <subfield code="c">2023</subfield>
    <subfield code="d">Q3</subfield>
  </datafield>
  <datafield tag="594" ind1=" " ind2=" ">
    <subfield code="a">3.0</subfield>
    <subfield code="b">2023</subfield>
  </datafield>
  <datafield tag="655" ind1=" " ind2="4">
    <subfield code="a">info:eu-repo/semantics/article</subfield>
    <subfield code="v">info:eu-repo/semantics/publishedVersion</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Arribas, M.</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
    <subfield code="0">(orcid)0000-0002-4426-6885</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Palacios, M.</subfield>
    <subfield code="0">(orcid)0000-0002-1374-4645</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Elipe, A.</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
    <subfield code="0">(orcid)0000-0001-5208-4494</subfield>
  </datafield>
  <datafield tag="710" ind1="2" ind2=" ">
    <subfield code="1">2005</subfield>
    <subfield code="2">595</subfield>
    <subfield code="a">Universidad de Zaragoza</subfield>
    <subfield code="b">Dpto. Matemática Aplicada</subfield>
    <subfield code="c">Área Matemática Aplicada</subfield>
  </datafield>
  <datafield tag="710" ind1="2" ind2=" ">
    <subfield code="1">2004</subfield>
    <subfield code="2">398</subfield>
    <subfield code="a">Universidad de Zaragoza</subfield>
    <subfield code="b">Dpto. Física Teórica</subfield>
    <subfield code="c">Área Física de la Tierra</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="g">135, 2 (2023), [23 pp.]</subfield>
    <subfield code="p">Celest. mech. dyn. astron.</subfield>
    <subfield code="t">Celestial Mechanics and Dynamical Astronomy</subfield>
    <subfield code="x">0923-2958</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2=" ">
    <subfield code="s">1597188</subfield>
    <subfield code="u">http://zaguan.unizar.es/record/124452/files/texto_completo.pdf</subfield>
    <subfield code="y">Versión publicada</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2=" ">
    <subfield code="s">1223528</subfield>
    <subfield code="u">http://zaguan.unizar.es/record/124452/files/texto_completo.jpg?subformat=icon</subfield>
    <subfield code="x">icon</subfield>
    <subfield code="y">Versión publicada</subfield>
  </datafield>
  <datafield tag="909" ind1="C" ind2="O">
    <subfield code="o">oai:zaguan.unizar.es:124452</subfield>
    <subfield code="p">articulos</subfield>
    <subfield code="p">driver</subfield>
  </datafield>
  <datafield tag="951" ind1=" " ind2=" ">
    <subfield code="a">2024-11-22-12:06:43</subfield>
  </datafield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">ARTICLE</subfield>
  </datafield>
</record>
</collection>