From GeV to PeV: Orbital Modulation and Wind-Regulated Ultrahigh-energy Emission in Cygnus X-3
astro-ph.HE
Submitted: 2026-10-08
Updated: 2026-10-08
Terminology
Sources
- Unveiling Multimessenger Emission from Hidden Cores of Microquasars
- Extreme Transients in Gamma Rays
- Near-IR and X-ray Variability of Cyg X-3: Evidence for a Compact IR Source and Complex Wind Structures
- The counterjet dominates the production of PeV photons from Cyg X-3
- Constraining the PeV gamma-ray emission zone of Cygnus X-3 with contemporaneous GeV timing and spectral observations
- Energy spectra of gamma-rays, electrons and neutrinos produced at proton-proton interactions in the very high energy regime
- Gemini/GNIRS infrared spectroscopy of the Wolf-Rayet stellar wind in Cygnus X-3
- Long-term study of the gamma-ray emission of Cygnus X-3 with MAGIC and Fermi-LAT
- The Disk-Wind-Jet Connection in the Black Hole H 1743-322
- On the role of the UV and X-ray radiation in driving a disk wind in X-ray binaries
- The proper motion and changing jet morphology of Cygnus X-3
- The lifetime of cosmic rays in the Milky Way
- An update on Fermi-LAT transients in the Galactic plane, including strong activity of Cygnus X-3 in mid-2020
- Microquasar Cygnus X-3 as the PeVatron powering the Cygnus Bubble
- Monte-Carlo simulations of photohadronic processes in astrophysics
- CRPropa 3.2 -- an advanced framework for high-energy particle propagation in extragalactic and galactic spaces
- The Temperature of the Cosmic Microwave Background
- Physical Properties of Wolf-Rayet Stars
- Black Hole Winds II: Hyper-Eddington Winds and Feedback
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