Interstellar scattering of the compact radio source 2005 + 403

Details Interstellar scattering of the compact radio source 2005 + 403 Interstellar scattering of the compact radio source 2005 + 403

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...349l..47m&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 349, Feb. 1, 1990, p. L47-L49.

Astronomy and Astrophysics

Astronomy

18

Electromagnetic Scattering, Interstellar Matter, Quasars, Radio Sources (Astronomy), Astronomical Models, Astronomical Spectroscopy, Red Shift, Very Long Base Interferometry

Scientific paper

Analysis of Mk III VLBI visibility amplitudes of the compact radio source 2005 + 403 shows an excess at baselines greater than a few diffractive scale lengths compared with that expected from formulas using ensemble-averaged quantities and power-law turbulence with quasi-Kolmogorov spectral indices. The data are in good agreement with the 1989 analysis of Goodman and Narayan, who find that measured visibility amplitudes correspond to the 'average' visibility regime, which differs significantly from the ensemble-averaged results for baselines much longer than one diffractive scale length.

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