<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
<record>
  <controlfield tag="001">2079</controlfield>
  <controlfield tag="005">20160701171658.0</controlfield>
  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ASTROimport-236</subfield>
  </datafield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Zorec, J.</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2005</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">Multi headed H alpha emission line profiles</subfield>
  </datafield>
  <datafield tag="520" ind1=" " ind2=" ">
    <subfield code="a">The Halpha emission line profile of Be stars have sometimes three or more peaks. The same type of line profile is also found in active objects with the B[e] phenomenon. In this contribution we discuss the formation of such emission line profiles in terms of rapidly expanding circumstellar rings. FULL TEXT IN SPANISH </subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a"> Arias, M. L.</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a"> Frémat, Y.</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="p">Boletin de la Asociacion Argentina de Astronomia La Plata Argentina</subfield>
    <subfield code="v">48</subfield>
    <subfield code="y">2005</subfield>
    <subfield code="c">263-266</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="2">
    <subfield code="a">http://esoads.eso.org/abs/2005BAAA...48..263Z</subfield>
  </datafield>
  <datafield tag="905" ind1=" " ind2=" ">
    <subfield code="a">published in</subfield>
  </datafield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">REFERD</subfield>
  </datafield>
</record>
</collection>