  In this work, we obtain uncharged\charged Kiselev-like black holes as a new
class of black hole solutions surrounded by perfect fluid in the context of
Rastall theory. Then, we study the specific cases of the uncharged\charged
black holes surrounded by regular matter like dust and radiation, or exotic
matter like quintessence, cosmological constant and phantom fields. By
comparing the Kiselev-like black hole solutions in Rastall theory with the
Kiselev black hole solutions in GR, we find an effective perfect fluid
behaviour for the black hole's surrounding field. It is shown that the
corresponding effective perfect fluid has interesting characteristic features
depending on the different ranges of the parameters in Rastall theory. For
instance, Kiselev-like black holes surrounded by regular matter in Rastall
theory may be considered as Kiselev black holes surrounded by exotic matter in
GR, or Kiselev-like black holes surrounded by exotic matter in Rastall theory
may be considered as Kiselev black holes surrounded by regular matter in GR.
