1 Ocak 2014 Konferans bildirisi Açık Erişim

Saha, Lab; Ergin, Tulun; Majumdar, Pratik; Bozkurt, Mustafa

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/99673</identifier>
  <creators>
    <creator>
      <creatorName>Saha, Lab</creatorName>
      <givenName>Lab</givenName>
      <familyName>Saha</familyName>
      <affiliation>Saha Inst Nucl Phys, Kolkata 700064, India</affiliation>
    </creator>
    <creator>
      <creatorName>Ergin, Tulun</creatorName>
      <givenName>Tulun</givenName>
      <familyName>Ergin</familyName>
      <affiliation>Tubitak Space Technol Res Inst, TR-06531 Ankara, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Majumdar, Pratik</creatorName>
      <givenName>Pratik</givenName>
      <familyName>Majumdar</familyName>
      <affiliation>Saha Inst Nucl Phys, Kolkata 700064, India</affiliation>
    </creator>
    <creator>
      <creatorName>Bozkurt, Mustafa</creatorName>
      <givenName>Mustafa</givenName>
      <familyName>Bozkurt</familyName>
      <affiliation>Bogazici Univ, Phys Dept, TR-34134 Istanbul, Turkey</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Locating The Tev Gamma-Rays From The Shell Regions Of Cassiopeia A</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2014</publicationYear>
  <dates>
    <date dateType="Issued">2014-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Conference paper</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/99673</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1017/S1743921313009927</relatedIdentifier>
  </relatedIdentifiers>
  <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">We have analyzed Chandra X-ray data from different parts of the shell of young supernova remnant (SNR) in the energy range of 0.7 - 8 keV. We observed that X-ray flux level varies over different shell regions of the source. Implications of X-ray observation will be discussed here. We also analyzed Fermi-LAT data in the energy range 0.5 - 50 GeV for the source. The differential spectrum obtained in this way fits with simple power-law. We also present here multi-wavelength modeling of the source considering archival radio and TeV data along with Chandra and Fermi-LAT data.</description>
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