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  <controlfield tag="005">20160701171709.0</controlfield>
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    <subfield code="a">10.1051/epjconf/201510106027</subfield>
    <subfield code="2">DOI</subfield>
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  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ASTROimport-855</subfield>
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  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Groenewegen, M. A. T.</subfield>
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  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2015</subfield>
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  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">The period distribution of Cepheids: a test of stellar evolution</subfield>
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  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">The period distributions of classical Cepheids in the Small and Large Magellanic Cloud are quite different. Using the TRILEGAL population synthesis code and a theoretical instability strip the ultimate aim is to understand these differences quantitatively. First results are presented for one area in the LMC using VMC NIR data. </subfield>
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  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a"> Girardi, L.</subfield>
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  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">European Physical Journal Web of Conferences</subfield>
    <subfield code="v">101</subfield>
    <subfield code="y">2015</subfield>
    <subfield code="c">06027</subfield>
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    <subfield code="a">http://esoads.eso.org/abs/2015EPJWC.10106027G</subfield>
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    <subfield code="a">published in</subfield>
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