  Recent results of Milagro, Tibet, ARGO-YBJ and IceCube experiments on the
small-scale anisotropy of Galactic cosmic rays (CRs) with energies from units
up to a few hundred TeV arise a question on a possible nature of the observed
phenomenon, as well as on the anisotropy of CRs at higher energies. An analysis
of a small-scale anisotropy of CRs with energies at around PeV registered with
the EAS MSU array presented in the article, reveals a number of regions with an
excessive flux. A typical size of the regions varies from 3 up to 12 degrees.
We study correlation of these regions with positions of potential astrophysical
sources of CRs and discuss a possible origin of the observed anisotropy.
