1 Ocak 2014 Konferans bildirisi Açık Erişim

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

Dublin Core

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  <dc:creator>Saha, Lab</dc:creator>
  <dc:creator>Ergin, Tulun</dc:creator>
  <dc:creator>Majumdar, Pratik</dc:creator>
  <dc:creator>Bozkurt, Mustafa</dc:creator>
  <dc:date>2014-01-01</dc:date>
  <dc:description>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.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/99673</dc:identifier>
  <dc:identifier>oai:zenodo.org:99673</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:title>Locating the TeV gamma-rays from the shell regions of Cassiopeia A</dc:title>
  <dc:type>info:eu-repo/semantics/conferencePaper</dc:type>
  <dc:type>publication-conferencepaper</dc:type>
</oai_dc:dc>