4FGL J1844.4–0306: High-energy Emission Likely from the Supernova Remnant G29.37 + 0.1

4FGL J1844.4–0306: High-energy Emission Likely from the Supernova Remnant G29.37 + 0.1

Very-high-energy (VHE) observations have revealed approximately 100 TeV sources in our Galaxy, and a significant fraction of them are under investigation to understand their origin. We report our study of one of them, HESS J1844−030. It is found to be possibly associated with the supernova remnant (...

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Bibliographic Details
Main Authors: Dong Zheng, Zhongxiang Wang, Xiao Zhang, Yang Chen, Yi Xing
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Supernova remnants
Pulsar wind nebulae
Gamma-ray sources
Online Access:https://doi.org/10.3847/1538-4357/ace10b

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