Constraining the PeV Gamma-Ray Emission Zone of Cygnus X-3 with Contemporaneous GeV Timing and Spectral Observations
Cygnus X-3 has recently been established as a variable ultra-high-energy gamma-ray source with photons detected up to 3.7 PeV. Its PeV activity is temporally correlated with Fermi-LAT GeV flares and may also be orbitally modulated, suggesting that the emission is produced within or close to the bina...
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| Hlavní autoři: | , , , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
IOP Publishing
2026-01-01
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| Edice: | The Astrophysical Journal Letters |
| Témata: | |
| On-line přístup: | https://doi.org/10.3847/2041-8213/ae6a9d |
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