VLBI data on TXS 2005+403 show refractive substructure from interstellar turbulence that cannot be explained by diffractive scattering alone and remains stable over nine years.
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Direct VLBI Detection of Interstellar Turbulence Imprint on a Quasar: TXS 2005+403
VLBI data on TXS 2005+403 show refractive substructure from interstellar turbulence that cannot be explained by diffractive scattering alone and remains stable over nine years.