Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978azh....55..299l&link_type=abstract
Astronomicheskii Zhurnal, vol. 55, Mar.-Apr. 1978, p. 299-306. In Russian.
Astronomy and Astrophysics
Astronomy
1
Background Radiation, Fine Structure, Galactic Radio Waves, Radio Sources (Astronomy), Milky Way Galaxy, Pulsars, Radiant Flux Density
Scientific paper
A uniform sample of radio sources from the Ohio survey is used to demonstrate an apparent correlation between these sources and extended features in the fine structure of Galactic radio-continuum radiation. A random distribution of radio sources in the Loop I and Loop II regions is assumed, and the probability of source projection into extended ridges of Galactic continuum radiation is evaluated. It is concluded that about 7% of the Ohio sources in the Loop I and Loop II regions with flux densities of at least 0.4 by 10 to the -26th power W/sq m per Hz belong to the Galaxy.
Larionov G. M.
Sidorenkov Valerii N.
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