The two phases of the interstellar medium - The electron density distribution in the Galactic disk

Details The two phases of the interstellar medium - The electron density distribution in the Galactic disk The two phases of the interstellar medium - The electron density distribution in the Galactic disk

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63.1111s&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 63, Nov.-Dec. 1986, p. 1111-1117. In Russian.

Astronomy and Astrophysics

Astronomy

1

Electron Density Profiles, Galactic Structure, Interstellar Matter, Milky Way Galaxy, Hydrogen Clouds, Nebulae, Pulsars, Space Density

Scientific paper

The current understanding of the diffuse interstellar medium is discussed. Dispersion measures of pulsars with known distances are used to construct a spatial distribution of the mean electron density for a diffuse interstellar medium in the Galactic disk. The distribution obtained corresponds to the concentration of the dispersive medium in the warm ionized H I component regions in the arms of the Galaxy.

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