A high-energy study of the supernova remnant G296.5+10.0

LAURA EPPENS; JORGE COMBI; ESTELA REYNOSO; FEDERICO GARCÍA; E. MESTRE; LEANDRO ABAROA; GUSTAVO E. ROMERO; PEDRO LUQUE ESCAMILLA; JOSEPH MARTI

MNRAS

Oxford University Press

Año: 2024 vol. 528

We report a detailed multi-wavelength study of the supernova remnant G296.5+10.0 using archival data from XMM–Newtonand Fermi-LAT complemented with ATCA observations. In the X-ray band, we performed an adaptive smoothing on the doublebackground subtracted images to construct an X-ray mosaic map with six individual observations. Below 2.0 keV, G296.5+10.0is asymmetrical, with the south-east side of the radio shell brighter than the south-west one. The spatially resolved X-rayspectral study confirms the thermal origin of the plasma, with enhanced metal abundances, probably arising from ejecta materialaccording to the H I and infrared (140 μm) distributions. In the γ -ray band, we analysed 14 years of accumulated Fermiobservations below 500 GeV via different fitting processes. To discuss the origin of the γ -ray emission, we compare the GeVresults with H I structures probably associated with the SNR and with the radio spectral indices found at various positionstowards the radio shell. Moreover, we identified diverse sources candidates to contribute γ -ray emissions observed. Also, wecalculated the lepto-hadronic spectral energy distribution of the remnant for synchrotron, inverse Compton, Bremsstrahlung,and proton–proton processes. The emission at low energies can be explained by electron-synchrotron radiation, with a weakmagnetic field of B = 25 μG, while the γ -ray data can be explained by hadronic interactions. Employing the reddening-distancemethod, we computed a distance of 1.4 kpc for the SNR, implying an age of 14 000 yr.