GeV Emission in the Region of the Supernova Remnant G51.26+0.11

The supernova remnant G51.26+0.11 was recently discovered and little is known about its properties environment. Using data from the Fermi Large Area Telescope we study GeV emission seen in direction of to constrain origin gamma-rays their possible relation this or a star-forming region. We also search for molecular gas region that could provide dense material production gamma-rays. By modeling multiwavelength spectrum radio derive particle populations produce several scenarios. rule out regions (such as G051.010+00.060) nearby emission. correspondence between gamma-ray morphologies supports scenario which cause flat spectral energy distribution observed at energies best fit by hadronic inverse Compton emission, while bremsstrahlung model cannot properly account fluxes under simple one-zone scenario. A pulsar wind nebula high-energy photons be ruled confirmed.