Speaker
Description
Detecting and studying galactic gamma-ray sources emitting very-high energy photons sheds light on the acceleration and propagation of cosmic rays presumably created in these sources. Currently, there are few sources emitting photons with energies exceeding 100 TeV. In this work we revisit the unidentified source MGRO J1908+063, initially detected by Milagro, using an updated H.E.S.S. dataset and analysis pipeline. The vicinity of the source contains a supernova remnant and pulsars as well as molecular clouds. This makes the identification of the primary source(s) of local cosmic rays as well as the nature of the gamma emission challenging, especially in light of the recent HAWC detection of the high energy tail of its spectrum. Exploiting the better angular resolution and spectral coverage of H.E.S.S. as compared to HAWC, we investigate the morphology of the source as well as its spectral properties and model different scenarios of gamma-ray production.
Keywords
pevatrons, galactic gamma rays, pulsars, supernova remnant, tev halos
| Subcategory | Experimental Results |
|---|---|
| Collaboration | H.E.S.S. |
