A contribution of the HAWC observatory to the TeV era in the high energy gamma-ray astrophysics: The case of the TeV-halos
Ramiro Torres-Escobedo, Hao Zhou, Eduardo de la Fuente for the HAWC Collaboration
SciPost Phys. Proc. 13, 029 (2023) · published 29 September 2023
- doi: 10.21468/SciPostPhysProc.13.029
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Proceedings event
21st International Symposium on Very High Energy Cosmic Ray Interactions
Abstract
We present a short overview of the TeV-Halos objects as a discovery and a relevant contribution of the High Altitude Water Çerenkov (HAWC) observatory to TeV astrophysics. We discuss history, discovery, knowledge, and the next step through a new and more detailed analysis than the original study in 2017. TeV-Halos will contribute to resolving the problem of the local positron excess observed on the Earth. To clarify the latter, understanding the diffusion process is mandatory.
Cited by 3
Authors / Affiliations: mappings to Contributors and Organizations
See all Organizations.- 1 Ramiro Torres-Escobedo,
- 1 Hao Zhou,
- 2 Eduardo de la Fuente Acosta
- 1 上海交通大学 / Shanghai Jiao Tong University [SJTU]
- 2 Universidad de Guadalajara / University of Guadalajara [UDG]
Funders for the research work leading to this publication