Two phases of the interstellar medium - The distribution of the scattering medium throughout the Galaxy

Details Two phases of the interstellar medium - The distribution of the scattering medium throughout the Galaxy Two phases of the interstellar medium - The distribution of the scattering medium throughout the Galaxy

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63..666s&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 63, July-Aug. 1986, p. 666-673. In Russian.

Astronomy and Astrophysics

Astronomy

6

Electron Density (Concentration), Interstellar Matter, Milky Way Galaxy, Pulsars, Radio Scattering, Stellar Radiation, Cosmic Plasma, Plasma Turbulence

Scientific paper

Attention is given to the distribution of electron density nonuniformities which are responsible for pulsar radio-emission scattering. Analysis of the observed and calculated dependences of pulsar pulse scattering in a statistically nonuniform medium did not reveal the correlation which is expected to exist between the mean and the rms value of electron density. It is suggested that hot ionized plasma is responsible for the scattering properties of the diffuse interstellar medium.

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