  We present intermediate resolution, wide wavelength coverage spectra for a
complete sample of 14 compact radio sources taken with the aim of investigating
the impact of the nuclear activity on the circumnuclear (ISM) in the early
stages of radio source evolution. We observe spatially extended line emission
(up to 20 kpc) in the majority of sources which is consistent with a quiescent
halo. In the nuclear apertures we observe broad, highly complex emission line
profiles. Multiple Gaussian modelling of the [O III]5007 line reveals 2-4
components which can have FWHM and blueshifts relative to the halo of up to
2000 km/s. We interpret these broad, blueshifted components as material in
outflow and discuss the kinematical evidence for jet-driven outflows.
Comparisons with samples in the literature show that compact radio sources
harbour more extreme nuclear kinematics than their extended counterparts, a
trend seen within our sample with larger velocities in the smaller sources. The
observed velocities are also likely to be influenced by source orientation with
respect to the observer's line of sight. Nine sources have associated HI
absorption. In common with the optical emission line gas, the HI profiles are
often highly complex with the majority of the detected components significantly
blueshifted, tracing outflows in the neutral gas. The sample has been tested
for stratification in the ISM (FWHM/ionisation potential/critical density) as
suggested by Holt et al. (2003) for PKS1345+12 but we find no significant
trends within the sample using a Spearman Rank analysis. This study supports
the idea that compact radio sources are young radio loud AGN observed during
the early stages of their evolution and currently shedding their natal cocoons
through extreme circumnuclear outflows.
