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- W2003192212 abstract "We report multi‐frequency VLBI observations of angular broadening of eight compact radio sources whose lines of sight pass through the galactic plane in Cygnus. We use the characteristics λ2 dependence of angular size to distinguish between intrinsic and scattered structure. Four of the eight sources have measured angular sizes larger than would be expected for sources with such spectra and exhibit a λ2 dependence of angular size. These results lead us to the conclusion that we have observed angular broadening for these four sources. The structures of the other four sources do not appear to be dominated by interstellar scattering. Our results indicate that scattering in the Cygnus region changes by a factor of 2–5 for sources separated by only a couple of degrees. With the exception of one of the sources, the observed angular broadening is confined within a few degrees of the galactic plane." @default.
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- W2003192212 date "1988-01-01" @default.
- W2003192212 modified "2023-10-14" @default.
- W2003192212 title "VLBI angular broadening measurements in the Cygnus region" @default.
- W2003192212 doi "https://doi.org/10.1063/1.37591" @default.
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