  Ground based long slit spectroscopic observations of the nuclear region of
NGC 5252, and Hubble Space Telescope (HST) Faint Object Spectrograph (FOS)
spectra of the nucleus and two bright knots located 0.36" NE and 0.31" SW from
it, show that the nuclear region exhibits the characteristics of a Liner with
exceptionally strong [OI] emission, all lines being broad (FWHM ~ 1100 km/s),
while the gas outside the nucleus has a typical Seyfert 2 spectrum with
relatively narrow lines (FWHM ~ 200-300 km/s). We suggest that all the emitting
gas is photoionized by the hidden non-thermal nuclear source detected through
near-infrared (Kotilainen & Prieto 1995) and X-ray (Cappi et al. 1996)
observations, the ionizing continuum, in the case of the central Liner, being
"filtered" by a matter-bounded highly ionized cloud, hidden from our view by
the same material obscuring the central continuum source.

Astrophysics