1 Ocak 2014 Konferans bildirisi Açık Erişim

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

Citation Style Language JSON

{
  "DOI": "10.1017/S1743921313009927", 
  "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.", 
  "author": [
    {
      "family": "Saha", 
      "given": " Lab"
    }, 
    {
      "family": "Ergin", 
      "given": " Tulun"
    }, 
    {
      "family": "Majumdar", 
      "given": " Pratik"
    }, 
    {
      "family": "Bozkurt", 
      "given": " Mustafa"
    }
  ], 
  "id": "99673", 
  "issued": {
    "date-parts": [
      [
        2014, 
        1, 
        1
      ]
    ]
  }, 
  "title": "Locating the TeV gamma-rays from the shell regions of Cassiopeia A", 
  "type": "paper-conference"
}