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arXiv · 2212.05713

MeV Gamma-Ray Source Contribution to the Inner Galactic Diffuse Emission

Naomi Tsuji·Yoshiyuki Inoue·Hiroki Yoneda·Reshmi Mukherjee·Hirokazu Odaka
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Abstract

The origin of the inner Galactic emission, measured by COMPTEL with a flux of $\sim 10^{-2} ~{\rm MeV~ cm}^{-2}~ {\rm s}^{-1}~ {\rm sr}^{-1}$ in the 1-30 MeV energy range from the inner Galactic region, has remained unsettled since its discovery. In this paper, we elaborate on a model of individual MeV gamma-ray sources unresolved by COMPTEL. This is conducted for sources crossmatched between the Swift-BAT and Fermi-LAT catalogs by interpolating the energy spectra in the hard X-ray and GeV gamma-ray ranges, as well as unmatched sources between the two catalogs. We find that the source contribution to the COMPTEL emission would be at least ~20%. Combined with the Galactic diffuse emission, which is not well constrained, the COMPTEL emission can be roughly reproduced in some cases.

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Naomi Tsuji, Yoshiyuki Inoue, Hiroki Yoneda, Reshmi Mukherjee, Hirokazu Odaka. 2022-12-12. MeV Gamma-Ray Source Contribution to the Inner Galactic Diffuse Emission. https://doi.org/10.3847/1538-4357%2Facab69

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