VLBI observations of TXS 0506+056 show a spine-sheath jet with aligned inner and perpendicular outer EVPAs plus a new superluminal component near the IceCube neutrino detection.
Title resolution pending
5 Pith papers cite this work, alongside 36 external citations. Polarity classification is still indexing.
5
Pith papers citing it
36
external citations · OpenAlex
years
2026 5representative citing papers
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.
Efficient neutrino production in blazar jets requires an external radiation field that strongly dominates the magnetic field (Y>>1), which radio constraints place near the broad-line region and only for uncommon jet acceleration or beaming conditions.
VLBI observations resolve NGC 7479's nucleus into two radio components separated by ~30 mas with an apparent change in separation over a decade, suggesting relativistic jet motion or nuclear wind shocks.
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.
citing papers explorer
-
Parsec-scale polarimetry and kinematics of a spine-sheath jet in the neutrino-blazar TXS 0506+056
VLBI observations of TXS 0506+056 show a spine-sheath jet with aligned inner and perpendicular outer EVPAs plus a new superluminal component near the IceCube neutrino detection.
-
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.
-
Locating the Production Sites of High-Energy Neutrinos in Blazar Jets
Efficient neutrino production in blazar jets requires an external radiation field that strongly dominates the magnetic field (Y>>1), which radio constraints place near the broad-line region and only for uncommon jet acceleration or beaming conditions.
-
Very Long Baseline Interferometry Search for Nuclear Radio Continuum Emission in the Barred Spiral Galaxy NGC 7479
VLBI observations resolve NGC 7479's nucleus into two radio components separated by ~30 mas with an apparent change in separation over a decade, suggesting relativistic jet motion or nuclear wind shocks.
-
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.