TY  - JOUR
AU  - HAWC Collaboration (Albert, A. et al
AU  - Salesa Greus, F.
PY  - 2021
DA  - 2021//
TI  - Evidence that Ultra-high-energy Gamma Rays Are a Universal Feature near Powerful Pulsars
T2  - Astrophys. J. Lett.
JO  - Astrophysical Journal Letters
SP  - L27 - 8pp
VL  - 911
IS  - 2
PB  - Iop Publishing Ltd
AB  - The highest-energy known gamma-ray sources are all located within 0.degrees 5 of extremely powerful pulsars. This raises the question of whether ultra-high-energy (UHE; >56 TeV) gamma-ray emission is a universal feature expected near pulsars with a high spin-down power. Using four years of data from the High Altitude Water Cherenkov Gamma-Ray Observatory, we present a joint-likelihood analysis of 10 extremely powerful pulsars to search for subthreshold UHE gamma-ray emission correlated with these locations. We report a significant detection (>3 sigma), indicating that UHE gamma-ray emission is a generic feature of powerful pulsars. We discuss the emission mechanisms of the gamma rays and the implications of this result. The individual environment, such as the magnetic field and particle density in the surrounding area, appears to play a role in the amount of emission.
SN  - 2041-8205
UR  - https://arxiv.org/abs/2101.07895
UR  - https://doi.org/10.3847/2041-8213/abf4dc
DO  - 10.3847/2041-8213/abf4dc
LA  - English
N1  - WOS:000642352500001
ID  - HAWCCollaborationAlbert+SalesaGreus2021
ER  -