  We performed a detailed study of the extended cool gas, traced by MgII
absorption [$W_r(2796)\geq0.3$~{\AA}], surrounding 14 narrow-line active
galactic nuclei (AGNs) at 0.12<z<0.22 using background quasar sight-lines. The
background quasars probe the AGNs at projected distances of $60\leq
D\leq265$~kpc. We find that, between $100\leq D\leq200$~kpc, AGNs appear to
have lower MgII gas covering fractions (0.09$^{+0.18}_{-0.08}$) than quasars
(0.47$^{+0.16}_{-0.15}$) and possibly lower than in active field galaxies
(0.25$^{+0.11}_{-0.09}$). We do not find a statistically significant azimuthal
angle dependence for the MgII covering fraction around AGNs, though the data
hint at one. We also study the `down-the-barrel' outflow properties of the AGNs
themselves and detect intrinsic NaID absorption in 8/8 systems and intrinsic
MgII absorption in 2/2 systems, demonstrating that the AGNs have significant
reservoirs of cool gas. We find that 6/8 NaID and 2/2 MgII intrinsic systems
contain blueshifted absorption with $\Delta v>50$ km/s, indicating outflowing
gas. The 2/2 intrinsic MgII systems have outflow velocities a factor of $\sim4$
higher than the NaID outflow velocities. Our results are consistent with
AGN-driven outflows destroying the cool gas within their halos, which
dramatically decreases their cool gas covering fraction, while star-burst
driven winds are expelling cool gas into their circumgalactic media (CGM). This
picture appears contrary to quasar--quasar pair studies which show that the
quasar CGM contains significant amounts of cool gas whereas intrinsic gas found
`down-the-barrel' of quasars reveals no cool gas. We discuss how these results
are complementary and provide support for the AGN unified model.
