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  <controlfield tag="001">1886</controlfield>
  <controlfield tag="005">20160701171655.0</controlfield>
  <datafield tag="024" ind1="7" ind2=" ">
    <subfield code="a">10.1007/BF00692128</subfield>
    <subfield code="2">DOI</subfield>
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  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ASTROimport-43</subfield>
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  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Pauwels, T.</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">1994</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Final tidal evolution of orbit-orbit resonances</subfield>
  </datafield>
  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">In this paper we describe a model for the tidal evolution of an orbit-orbit resonance between two satellites of the same planet. We let the system evolve till infinity or until the resonance is destroyed. We find that there are asymptotic values for the eccentricities and inclinations. We list the possible final stages that a resonance can achieve, we give a few examples, and finally we discuss the limitations of the model and its possible applications to real systems. </subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">Celestial Mechanics and Dynamical Astronomy</subfield>
    <subfield code="v">59</subfield>
    <subfield code="y">1994</subfield>
    <subfield code="c">101-127</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="2">
    <subfield code="a">http://esoads.eso.org/abs/1994CeMDA..59..101P</subfield>
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  <datafield tag="905" ind1=" " ind2=" ">
    <subfield code="a">published in</subfield>
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  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">REFERD</subfield>
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