The Cygnus Bubble's ultra-high-energy gamma-ray emission above 400 TeV is physically more consistent with a microquasar halo around Cygnus X-3 than with the Cygnus OB2 star-forming region.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
representative citing papers
Time-dependent cosmic ray electron spectra in a simulated galactic disk match steady-state solutions up to 500 GeV but become steeper and more disk-confined at higher energies due to recent injections.
End-to-end CTAO simulations show that 50h observations will detect Geminga and Monogem TeV halos at 13–30σ and constrain injection index to Δγ₁≈0.2, magnetic field to ΔB≈2μG, and SDZ size for Monogem.
citing papers explorer
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Microquasar Cygnus X-3 as the PeVatron powering the Cygnus Bubble
The Cygnus Bubble's ultra-high-energy gamma-ray emission above 400 TeV is physically more consistent with a microquasar halo around Cygnus X-3 than with the Cygnus OB2 star-forming region.
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Steady-State or Not? The Evolution of Cosmic Ray Electron Spectra in Galaxies
Time-dependent cosmic ray electron spectra in a simulated galactic disk match steady-state solutions up to 500 GeV but become steeper and more disk-confined at higher energies due to recent injections.
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Geminga and Monogem in the CTAO Era: Probing TeV Halos and Cosmic-Ray Transport
End-to-end CTAO simulations show that 50h observations will detect Geminga and Monogem TeV halos at 13–30σ and constrain injection index to Δγ₁≈0.2, magnetic field to ΔB≈2μG, and SDZ size for Monogem.