A lepto-hadronic reconnection model with an emission blob moving from 2 to 4 pc can match the neutrino and TeV gamma-ray sequence of the TXS 0506+056 2017 flare.
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Multi-messenger emission from magnetic reconnection in blazar jets: the case of TXS 0506+056
A lepto-hadronic reconnection model with an emission blob moving from 2 to 4 pc can match the neutrino and TeV gamma-ray sequence of the TXS 0506+056 2017 flare.