Possible correlation between discrete radio sources and fine structure of the galactic continuum radiation

A considerable correlation between the radio sources of the Ohio survey of the sky and the extended features of fine structure of the continuum radiation of the Galaxy was obtained as a result of a statistical investigation. The probability of projection of radiosources in loop 1 and loop 2 regions on the extended ''ridges'' of continuum galactical radio emission has been evaluated in the suggestion of a random distribution of these sources. It is shown that about 7 per cent of the radio sources of the Ohio Survey with fluxes S (>=) 0.4x10-2 W/m2 Hz may belong to the Galaxy