在高能伽玛射线天体物理学中,HAWC天文台对TeV时代的贡献:TeV晕的情况

Ramiro Torres-Escobedo, Hao Zhou, Eduardo de la Fuente Acosta
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引用次数: 0

摘要

我们简要介绍了TeV-晕天体的发现以及高空水Çerenkov (HAWC)天文台对TeV天体物理学的相关贡献。我们通过比2017年的原始研究更详细的新分析来讨论历史,发现,知识和下一步。tev光晕将有助于解决在地球上观测到的局部正电子过剩的问题。要阐明后者,必须了解扩散过程。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A contribution of the HAWC observatory to the TeV era in the high energy gamma-ray astrophysics: The case of the TeV-halos
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.
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