1 Ocak 1994 Dergi makalesi Açık Erişim

DENIZMAN, L; AK, T; KOKTAY, T; SAYGAC, T; KOCER, D

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/100945</identifier>
  <creators>
    <creator>
      <creatorName>DENIZMAN, L</creatorName>
      <givenName>L</givenName>
      <familyName>DENIZMAN</familyName>
    </creator>
    <creator>
      <creatorName>AK, T</creatorName>
      <givenName>T</givenName>
      <familyName>AK</familyName>
    </creator>
    <creator>
      <creatorName>KOKTAY, T</creatorName>
      <givenName>T</givenName>
      <familyName>KOKTAY</familyName>
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    <creator>
      <creatorName>SAYGAC, T</creatorName>
      <givenName>T</givenName>
      <familyName>SAYGAC</familyName>
    </creator>
    <creator>
      <creatorName>KOCER, D</creatorName>
      <givenName>D</givenName>
      <familyName>KOCER</familyName>
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  </creators>
  <titles>
    <title>On The Further Observations Of B-E/Shell Star-V-923-Aql</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>1994</publicationYear>
  <dates>
    <date dateType="Issued">1994-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/100945</alternateIdentifier>
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  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.81043/aperta.100944</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.81043/aperta.100945</relatedIdentifier>
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  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">V 923 Aql is one of the candidate B-e stars to be a binary star. In this research, optical and near-infrared spectral measurements of V 923 Aql is presented. V 923 Aql presents variable H Balmer line profiles with shell components. H alpha profiles present R/V, E/C and radial velocity variation. Shell parameters of the envelope are calculated.</description>
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