<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
<record>
  <controlfield tag="001">2505</controlfield>
  <controlfield tag="005">20160701171706.0</controlfield>
  <datafield tag="024" ind1="7" ind2=" ">
    <subfield code="a">10.1017/S1743921305009609</subfield>
    <subfield code="2">DOI</subfield>
  </datafield>
  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ASTROimport-662</subfield>
  </datafield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Frémat, Y.</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2004</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Chemical analysis of a triple system of A-type stars</subfield>
  </datafield>
  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">Components of multiple systems generally originate from the same protostellar environment. Their similarities or differences in surface chemical composition therefore relates to their individual evolutionary paths (stellar evolution, rotation) and the possible influence of a close companion. </subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a"> Lampens, P.</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a"> Hensberge, H.</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">The A-Star Puzzle</subfield>
    <subfield code="v">224</subfield>
    <subfield code="y">2004</subfield>
    <subfield code="c">701-705</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="2">
    <subfield code="a">http://esoads.eso.org/abs/2004IAUS..224..701F</subfield>
  </datafield>
  <datafield tag="905" ind1=" " ind2=" ">
    <subfield code="a">published in</subfield>
  </datafield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">NONREF</subfield>
  </datafield>
</record>
</collection>