  Two Component Advective Flow (TCAF) successfully explains the spectral and
tem- poral properties of outbursting or persistent sources. Images of static
TCAF with Compton cloud or CENtrifugal pressure supported Boundary Layer
(CENBOL) due to gravitational bending of photons have been studied before. In
this paper, we study time dependent images of advective flows around a
Schwarzschild black hole which include cooling effects due to Comptonization of
soft photons from a Keplerian disks well as the self-consistently produced jets
and outflows. We show the overall image of the disk-jet system after convolving
with a typical beamwidth. A long exposure image with time dependent system need
not show the black hole horizon conspicuously, un- less one is looking at a
soft state with no jet or the system along the jet axis. Assuming these
disk-jet configurations are relevant to radio emitting systems also, our
results would be useful to look for event horizons in high accretion rate
Supermassive Black Holes in Seyfert galaxies, RL Quasars.
