The Fermi-LAT GeV excess as a tracer of stellar mass in the Galactic bulge
Nov 13, 2017
10 pages
Published in:
- Nature Astron. 2 (2018) 10, 819-828
- Published: Aug 6, 2018
e-Print:
- 1711.04778 [astro-ph.HE]
DOI:
- 10.1038/s41550-018-0531-z (publication)
View in:
Citations per year
Abstract: (Springer)
An anomalous emission component at energies of a few gigaelectronvolts and located towards the inner Galaxy is present in the Fermi-LAT data. At present, the two most promising explanations are the annihilation of dark matter particles or the presence of a large population of unresolved point sources, most probably millisecond pulsars, at the Galactic Centre. Here, we report an analysis of the excess characteristics using almost eight years of Pass 8 ULTRACLEAN Fermi-LAT data with SkyFACT—a tool that combines image reconstruction with template-fitting techniques. We find that an emission profile that traces stellar mass in the boxy and nuclear bulge is preferred over conventional dark matter profiles. A model including the bulge is favoured over a model with dark matter at 16σ.Note:
- 7 pages, 4 figures, 1 table + supplemental material
- galaxy
- GLAST
- nucleus
- dark matter: relic density
- statistical
- mass ratio
- numerical calculations
References(89)
Figures(8)