Magnetic reconnection in NGC 1275's jet produces plasmoids that power the observed TeV flares, with leptonic emission favored but hadronic possible under compressed gas conditions.
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A Model for Magnetic Reconnection as the Origin of TeV Outbursts from NGC 1275
Magnetic reconnection in NGC 1275's jet produces plasmoids that power the observed TeV flares, with leptonic emission favored but hadronic possible under compressed gas conditions.