Searching for GeV gamma-ray emission from the bulge of M31

Abstract

The three major large-scale, diffuse $\gamma$-ray structures of the Milky Way are the Galactic disk, a bulge-like GeV excess towards the Galactic center, and the Fermi bubble. Whether such structures can also be present in other normal galaxies remains an open question. M31, as the nearest massive normal galaxy, holds promise for spatially-resolving the $\gamma$-ray emission. Based on more than 8 years of Fermi-LAT observations, we use (1) disk, (2) bulge, and (3) disk-plus-bulge templates to model the spatial distribution of the $\gamma$-ray emission from M31. Among these, the disk-plus-bulge template delivers the best-fit, in which the bulge component has a TS value 25.7 and a photon-index of $2.57\pm 0.17$, providing strong evidence for a centrally-concentrated gamma-ray emission from M31, that is analogous to the Galactic center excess. The total 0.2-300 GeV gamma-ray luminosity from this bulge component is $(1.16\pm 0.14)\times 10^{38}erg{s}^{-1}$, which would require $\sim 1.5\times 10^5$ millisecond pulsars, if they were the dominant source. We also search for a Fermi bubble-like structure in M31 using the full dataset (pass8), but no significant evidence is found. In addition, a likelihood analysis using only photons with the most accurate reconstructed direction (i.e., PSF3-only data) reveals a 4.8 $\sigma$ point-like source located at $\sim$ 10kpc to the northwest of the M31 disk, with a luminosity of $(0.97\pm 0.27)\times 10^{38}erg{s}^{-1}$ and a photon-index of $2.31\pm 0.18$. Lacking of a counterpart on the southeast side of the disk, the relation between this point-like source and a bubble-like structure remains elusive.

19 pages, 8 figures, accepted by RAA

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Cited by in corpus (5)

• Exploring A Cosmic-Ray Origin of the Multi-wavelength Emission in M31
• XMM-Newton RGS spectroscopy of the M31 bulge. I: Evidences for a past AGN half a million years ago
• Gamma-ray image reconstruction of the Andromeda galaxy
• Optimal observing strategies for velocity-suppressed dark matter annihilation
• M31 nucleus: molecular and ionised gas content upper limits