The problem of the galactic halo

Details The problem of the galactic halo The problem of the galactic halo

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976izssr..40..522b&link_type=abstract

(Vsesoiuznaia Konferentsiia po Fizike Kosmicheskikh Luchei, Samarkand, Uzbek SSR, Oct. 29-31, 1975.) Akademiia Nauk SSSR, Izvest

Astronomy and Astrophysics

Astronomy

Electron Energy, Galactic Structure, Halos, Milky Way Galaxy, Radio Astronomy, Astronomical Models, Cosmic Rays, High Energy Electrons

Scientific paper

The size of the halo of the Milky Way Galaxy is investigated by calculating the number of radio-emitting electrons along the line of sight. The inhomogeneity of the distribution of these electrons, which apparently are responsible for the radio background, is computed by means of a cosmic-ray diffusion model describing particle motion in tangled magnetic fields. Three electron energy regions are discovered: the high-energy region, the low-energy region, and the intermediate energy region. Low-energy electrons are shown to be the major component of the halo.

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