Draft:Gamma-ray binary
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Gamma-ray binary is a class of high-mass binary star system that emits the majority of its radiation at gamma-ray wavelengths, typically in the form of non-thermal emission peaking above 1 MeV.[1] One example is LMC P3
See also
Reference
- ^ "Fermi Gamma-ray Space Telescope: Exploring the Extreme Universe". fermi.gsfc.nasa.gov. Retrieved 2025-12-21.
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