Locating the TeV gamma-rays from the shell regions of Cassiopeia A

Date

2014-01-01

Author

Saha, Lab
Ergin, Tülün
Majumdar, Pratik
Bozkurt, Mustafa

Metadata

Show full item record

This work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.

Item Usage Stats

1
views

2
downloads

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.

Subject Keywords

Cassiopeia A, X-rays, Observations

URI

https://hdl.handle.net/11511/32851

Collections

Department of Physics, Conference / Seminar