Explicit algebraic expressions for cosmic ray electron number density as a function of position and energy are derived for axisymmetric source distributions in galaxies.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
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Multi-scale radio observations of 15 local U/LIRGs decompose emission to show nuclear components contribute ~50% on average while diffuse SF-related emission dominates ~80% of total power, with radio excess linked to AGN rather than boosted star formation.
citing papers explorer
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The Distribution of Cosmic Ray Electrons in Star-Forming Galaxies
Explicit algebraic expressions for cosmic ray electron number density as a function of position and energy are derived for axisymmetric source distributions in galaxies.
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The PARADIGM Project II: Characterising Nuclear and Diffuse Radio Components in Local U/LIRGs
Multi-scale radio observations of 15 local U/LIRGs decompose emission to show nuclear components contribute ~50% on average while diffuse SF-related emission dominates ~80% of total power, with radio excess linked to AGN rather than boosted star formation.