  The primary cosmic ray sources are searched by means of CHRONOTRON - KLARA
separate array of the P.N. Lebedev Physical Institute Tien Shan station. It was
done on the base of 35 millions observed PCR extensive air showers from
5x10**13 to 5x10**14 eV energies. The data analysis was carried on the method
of the direct selection of local areas in equatorial coordinates where the
deviation of event numbers exceeded the definite value from normal Gaussian
standard. These directions are compared with other arrays observed results and
with coordinates of astrophysical sources.
