Revision of the GeV γ-Ray Emission in the Region of HESS J1813-178 with Fermi-LAT
HESS J1813-178 is one of the brightest and most compact TeV γ -ray sources, and whether its γ -ray emission is associated with supernova remnant (SNR), pulsar wind nebula (PWN), or young stellar cluster (YSC) is still under debate. By analyzing the GeV γ -ray data in the field of HESS J1813-178 usin...
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| Hlavní autoři: | , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
IOP Publishing
2024-01-01
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| Edice: | The Astrophysical Journal |
| Témata: | |
| On-line přístup: | https://doi.org/10.3847/1538-4357/ad2ae1 |
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