Diffusive spreading of dynamo fields into turbulent exteriors reverses the usual decay ordering, allowing quadrupole toroidal components to decay slower than dipoles and confining fields within a magnetosphere whose synchrotron signatures are potentially observable.
Monthly Notices of the Royal Astronomical Society , volume =
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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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Magnetic field spreading from stellar and galactic dynamos into the exterior
Diffusive spreading of dynamo fields into turbulent exteriors reverses the usual decay ordering, allowing quadrupole toroidal components to decay slower than dipoles and confining fields within a magnetosphere whose synchrotron signatures are potentially observable.
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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.