The study of 3C 219 quasar and its surroundings was carried out. The distribution of galaxies, galaxies systems, and quasars inside the surface within a 360-minute radius is the same everywhere. It turned out that the distribution in the 3C 219 is homogeneous.

A sample of 289 compact radio sources selected from the 7C Catalogue, covering an area of 0.097 steradian, was surveyed at 102 Mhz by the scintillation method. The observations show that the sizes of these sources are less than 0.1” and their flux densities do not exceed 2 Yn. These sources are identified with objects from the FIRST catalogue of radio sources. 99 of these objects have scintillations and have no neighbor in the surrounding 5’. 34 of those 99 are identified with objects on the POSS within 10”×10” areas. 17 of the last 34 are closer to identified POSS objects (within 2”×2” areas). So we suppose that these 17 radio sources are clearly identified with optical sources. Most of them are probably bright quasars. The other 17 will not be discussed here, as we didn’t succeed in their optical identification. There are no POSS objects brighter than 21m in the close surroundings of the remaining 65 radio sources. We have started optical observations of areas close to those 65 objects with the 2.6-m telescope of the Byurakan observatory. Up to now 15 areas were observed. In 5 cases optical objects were found fainter than 22m — 24m within 3” of the compact radio sources (one example is shown in Fig. 1). We are sure that there are no optical objects brihgter than 25m that may be identified with the remaining 10 objects. Those five identifications give us an opportunity to suppose that they are remote quasars. More powerful telescopes than the 2.6-m are needed to perform photometric and spectral observations of similar objects in order to prove our suggestion.