Stellar atmospheres produce a sub-dominant Galactic diffuse gamma-ray and neutrino background that is negligible at 1 TeV and below IceCube limits but becomes an irreducible local component above 10 TeV.
Hudson, et al.,No evidence for a dynamo in the con- vection zone of a rapidly rotating red giant, Mon
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Galactic Diffuse Gamma-Ray and Neutrino Emission from Cosmic-Ray Interactions in Stellar Atmospheres
Stellar atmospheres produce a sub-dominant Galactic diffuse gamma-ray and neutrino background that is negligible at 1 TeV and below IceCube limits but becomes an irreducible local component above 10 TeV.