Anisotropic Interstellar Scattering Towards The Cygnus Region

Details Anisotropic Interstellar Scattering Towards The Cygnus Region Anisotropic Interstellar Scattering Towards The Cygnus Region

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...192.4612d&link_type=abstract

American Astronomical Society, 192nd AAS Meeting, #46.12; Bulletin of the American Astronomical Society, Vol. 30, p.879

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We have observed several extragalactic sources seen towards the Cygnus region. These sources are angularly broadened by radio-wave scattering due to interstellar turbulence. The angular broadening is anisotropic and the anisotropy seems to be frequency independent. We report on attempts to measure the power law index, the inner scale, and refractive effects in these data. We also discuss the implications of these measurements for the form of the turbulence spectrum.

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