  The radiation fields external to the jets and originating from within a few
parsecs from the black hole, are discussed in this paper. They are the direct
radiation from an accretion disk in symbiosis with jets, the radiation field
from the broad line region (BLR) surrounding the accretion disk, and the
infrared radiation from a dusty torus. The jet/disk symbiosis modifies the
energetics in the central parsec of AGN such that for a given accretion rate, a
powerful jet would occur at the expense of the disk luminosity, and
consequently the disk would less efficiently ionize the BRL clouds or heat the
dust in the torus, thereby affecting potentially important target photon fields
for interactions of gamma-rays, accelerated electrons and protons along the
jet.
  Motivated by unification schemes of active galactic nuclei, we briefly review
the evidence for the existence of broad line regions and small-scale dust tori
in BL Lacs and Fanaroff-Riley Class I (FR-I) radio galaxies. We propose that an
existing jet-accretion disk symbiosis can be extrapolated to provide a large
scale-symbiosis between other important dusty constituents of the blazar/FR-I
family. In the present paper, we discuss in the context of this symbiosis
interactions of GeV and TeV gamma-rays produced in the jet with the various
radiation fields external to the jet in quasars and blazars, taking account the
anisotropy of the radiation.
