VLBI monitoring reveals a 21c apparent speed in TXS 0506+056, interpreted as evidence for a stratified jet with Gamma>20 spine that accounts for neutrino production and radio flare timing.
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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
SKA-VLBI can deliver high-sensitivity milliarcsecond imaging and polarimetry of faint blazars to constrain models of high-energy photon and neutrino emission in AGN jets.
SKA VLBI surveys of the Southern sky will support geodesy with a Southern network, increase compact source density for calibration, extend the celestial reference frame, and enable high-precision astrometry for astrophysics.
citing papers explorer
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A hidden ultra-relativistic spine in the jet of a neutrino-associated blazar
VLBI monitoring reveals a 21c apparent speed in TXS 0506+056, interpreted as evidence for a stratified jet with Gamma>20 spine that accounts for neutrino production and radio flare timing.
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SKA-VLBI Probes of High-energy Emission Processes in Relativistic Jets
SKA-VLBI can deliver high-sensitivity milliarcsecond imaging and polarimetry of faint blazars to constrain models of high-energy photon and neutrino emission in AGN jets.
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SKA VLBI survey of the Southern sky for astrometry, geodesy, and astrophysics
SKA VLBI surveys of the Southern sky will support geodesy with a Southern network, increase compact source density for calibration, extend the celestial reference frame, and enable high-precision astrometry for astrophysics.