  We have obtained with the LBT Telescope AO system Near-Infrared camera PISCES
images of the inner-shell of the nebula around the luminous blue variable star
P Cygni in the [Fe II] emission line at 1.6435 {\mu}m. We have combined the
images in order to cover a field of view of about 20" around P Cygni thus
providing the high resolution (0".08) 2-D spatial distribution of the
inner-shell of the P Cygni nebula in [Fe II]. We have identified several
nebular emission regions which are characterized by an S/N>3. A comparison of
our results with those available in the literature shows full consistency with
the finding by Smith & Hartigan (2006) which are based on radial velocity
measurements and their relatively good agreement with the extension of emission
nebula in [NII] {\lambda}6584 found by Barlow et al. (1994). We have clearly
detected extended emission also inside the radial distance R=7".8 and outside
R=9".7 which are the nebular boundaries proposed by Smith & Hartigan (2006).
New complementary spectroscopic observations to measure radial velocities and
to derive the 3-D distribution of P Cygni nebula are planned.

Solar and Stellar Astrophysics;Instrumentation and Methods for Astrophysics