The radio/IR/gamma-ray correlation in galaxies is an emergent geometric property of line-of-sight integration through radially structured discs, not a signature of local cosmic-ray calorimetry.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Observational evidence links obscured super-Eddington accretion to slower precessing jets in stellar-mass compact object systems, contrasting with fixed fast jets in low-density environments.
citing papers explorer
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Geometry, Not Calorimetry, Drives the Radio/Infrared/Gamma-Ray Correlation
The radio/IR/gamma-ray correlation in galaxies is an emergent geometric property of line-of-sight integration through radially structured discs, not a signature of local cosmic-ray calorimetry.
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The link between obscured accretion and mildly relativistic precessing jets
Observational evidence links obscured super-Eddington accretion to slower precessing jets in stellar-mass compact object systems, contrasting with fixed fast jets in low-density environments.