Improved estimates of interstellar scattering through the inner galaxy

Details Improved estimates of interstellar scattering through the inner galaxy Improved estimates of interstellar scattering through the inner galaxy

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.234..853p&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 234, Oct. 15, 1988, p. 853-862.

Astronomy and Astrophysics

Astronomy

4

Electromagnetic Scattering, Interstellar Matter, Milky Way Galaxy, Planetary Systems, Radio Sources (Astronomy), Galactic Nuclei, Scintillation, Very Long Base Interferometry

Scientific paper

A total of forty-one radio sources near the galactic plane were studied for interplanetary scintillations at 1420 and 327 MHz. Of the sources, eight showed scintillations at 1420 MHz and one showed scintillations at 327 MHz. It is suggested that the most likely explanation for the abscence of scintillations at 327 MHz is angular broadening of radio sources due to interstellar scattering.

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