Investigating -ray halos around three HAWC bright sources in Fermi-LAT data
arXiv:2012.05932 · doi:10.1103/PhysRevD.104.103002
Abstract
Numerous extended sources around Galactic pulsars have shown significant -ray emission from GeV to TeV energies, revealing hundreds of TeV energy electrons scattering off of the underlying photon fields through inverse Compton scattering (ICS). HAWC TeV gamma-ray observations of few-degree extended emission around the pulsars Geminga and Monogem, and LAT GeV emission around Geminga, suggest that systems older than 100 kyr have multi-TeV propagating beyond the SNR-PWN system into the interstellar medium. Following the discovery of few -ray sources by HAWC at energies E~TeV, we investigate the presence of an extended -ray emission in Fermi-LAT data around the three brightest sources detected by HAWC up to 100 TeV. We find an extended emission of deg around eHWC J1825-134 and deg eHWC J1907+063. The analysis with ICS templates on Fermi-LAT data point to diffusion coefficient values which are significantly lower than the average Galactic one. When studied along with HAWC data, the -ray Fermi-LAT data provide invaluable insight into the very high-energy electron and positron parent populations.
arXiv comment18 pages and 11 figures. Phys.Rev.D 104 (2021) 10, 103002
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