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  <controlfield tag="001">2484</controlfield>
  <controlfield tag="005">20160701171706.0</controlfield>
  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ASTROimport-641</subfield>
  </datafield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Blomme, R.</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2002</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Stellar Winds of Early-Type Stars</subfield>
  </datafield>
  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">Previous work on IRAS observations showed inhomogen- eities ("clumping") to be present in the wind of some early- type stars. To study this in more detail, we obtained ISOPHOT data at 60, 90 and 160 m for 1 LBV, 2 B-type stars and 5 Wolf-Rayets. The ISOPHOT data consist of P32 oversampled maps, which show a strong and highly structured background (infrared cirrus) on which the weak signal of the star is super- posed. The data still need to be reduced and corrected for the background before fluxes can be derived. </subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a"> Runacres, M. C.</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">Photometric Mapping with ISOPHOT using the "P32" Astronomical Observation Template</subfield>
    <subfield code="v">482</subfield>
    <subfield code="y">2002</subfield>
    <subfield code="c">67</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="2">
    <subfield code="a">http://esoads.eso.org/abs/2002ESASP.482...67B</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>
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