Speaker
Dr
Emmanuel Moulin
Description
The H.E.S.S. array of imaging atmospheric telescopes is observing the Galactic Center since more that 20 years. The H.E.S.S. collaboration carried out deep very-high-energy (VHE, E>100 GeV) gamma-ray observations in a 25 degree squared region near the Galactic centre devised to reach the best sensitivity to VHE gamma-ray diffuse emission. We report here on the detection by H.E.S.S. of a VHE emission in the TeV energy regime coincident with the base of the Fermi Bubbles’ emission detected in Fermi-LAT observations. Possible emissions scenarios are discussed.
| Collaboration(s) | H.E.S.S. |
|---|