The distribution profile of a scattering medium in the Galaxy

Details The distribution profile of a scattering medium in the Galaxy The distribution profile of a scattering medium in the Galaxy

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..409b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, May 1988, p. 409-416. In Russian. In Russian. In Russian. In Ru

Astronomy and Astrophysics

Astronomy

2

Galactic Nuclei, Milky Way Galaxy, Radio Scattering, Interstellar Space, Pulsars

Scientific paper

The distribution profile of a scattering medium in the inner regions of the Galactic disk is constructed from pulsar radio-emission scattering observations using the 'space tomography' method. In a local region of the interstellar medium at distances over 100 pc in the vicinity of the sun, an increase is found in the turbulence intensity. An oscillating distribution component is found as well as one that is monotonically increasing toward the Galactic center.

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