Observation of Gamma Rays up to 320 TeV from the Middle-aged TeV Pulsar Wind Nebula HESS J1849−000
Gamma rays from HESS J1849−000, a middle-aged TeV pulsar wind nebula (PWN), are observed by the Tibet air shower array and the muon detector array. The detection significance of gamma rays reaches 4.0 σ and 4.4 σ levels above 25 TeV and 100 TeV, respectively, in units of the Gaussian standard deviat...
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Fformat: | Erthygl |
Iaith: | English |
Cyhoeddwyd: |
IOP Publishing
2023-01-01
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Cyfres: | The Astrophysical Journal |
Pynciau: | |
Mynediad Ar-lein: | https://doi.org/10.3847/1538-4357/acebce |