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  <controlfield tag="001">2734</controlfield>
  <controlfield tag="005">20160701171710.0</controlfield>
  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ASTROimport-891</subfield>
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  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Van de Steene, G.</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2014</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">A Herschel study of the Helix nebula</subfield>
  </datafield>
  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">The Herschel Guaranteed Time Key Project “MESS” (Mass loss of Evolved StarS) has observed a wide variety of evolved stellar objects in spectroscopic and photometric mode using both the PACS and SPIRE instruments on board the Herschel satellite. The aims of the project are to study the nebular morphology at far infrared wavelengths, the mass loss history of the central star, and the properties of the dust that was formed in the ejecta. In the poster we presented the results of the Herschel PACS and SPIRE imaging of the dust shell of the Helix planetary nebula NGC 7293. </subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">Asymmetrical Planetary Nebulae VI Conference</subfield>
    <subfield code="y">2014</subfield>
    <subfield code="c">108</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="2">
    <subfield code="a">http://esoads.eso.org/abs/2014apn6.confE.108V</subfield>
  </datafield>
  <datafield tag="905" ind1=" " ind2=" ">
    <subfield code="a">published in</subfield>
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  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">NONREF</subfield>
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