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.
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4 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 4years
2026 4verdicts
UNVERDICTED 4representative citing papers
3D force-free simulations demonstrate that FRBs excite Alfvén waves leading to nonlinear attenuation within 10-100 magnetar radii in quiescent fields and at larger radii in relativistic outflows.
A theoretical model in which monster radiative shocks launched by magnetar disturbances generate self-regulated GHz radio precursors that explain FRB activity from SGR 1935+2154 with sub-millisecond duration and specific energy scaling.
Force-free simulations confirm that fast magnetosonic waves undergo efficient parametric decay into secondary FMS and Alfvén waves, producing a broad spectrum and continued energy drain even after equipartition.
citing papers explorer
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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.
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Damping of Fast Radio Bursts in the Inner Magnetospheres of Magnetars
3D force-free simulations demonstrate that FRBs excite Alfvén waves leading to nonlinear attenuation within 10-100 magnetar radii in quiescent fields and at larger radii in relativistic outflows.
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Radio precursors of monster shocks: a mechanism for fast radio bursts from SGR 1935+2154
A theoretical model in which monster radiative shocks launched by magnetar disturbances generate self-regulated GHz radio precursors that explain FRB activity from SGR 1935+2154 with sub-millisecond duration and specific energy scaling.
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Nonlinear Decay of Fast Magnetosonic Waves through Weak Turbulence: Force-Free Electrodynamics Simulations
Force-free simulations confirm that fast magnetosonic waves undergo efficient parametric decay into secondary FMS and Alfvén waves, producing a broad spectrum and continued energy drain even after equipartition.