Investigating the region of 3C 397 in High Energy Gamma rays

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2017-02-24
Bhattacharjee, Pooja
Majumdar, Pratik
Ergin, Tülün
Saha, Lab
Joarder, Partha S.
We investigate the supernova remnant (SNR) 3C 397 and its neighboring pulsar PSR J1906+0722 in high energy gamma rays by using nearly six years of archival data of Large Area Telescope on board Fermi Gamma Ray Space Telescope (Fermi-LAT). The off-pulse analysis of gamma-ray flux from the location of PSR J1906+0722 reveals an excess emission which is found to be very close to the radio location of 3C 397. Here, we present the preliminary results of this gamma-ray analysis of 3C 397 and PSR J1906+0722.
Citation Formats
P. Bhattacharjee, P. Majumdar, T. Ergin, L. Saha, and P. S. Joarder, “Investigating the region of 3C 397 in High Energy Gamma rays,” 2017, vol. 12, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/44097.