IFU spectroscopy of southern PNe: III
  In this paper we describe integral field spectroscopic observations of four
southern Galactic Planetary Nebulae (PNe), M3-4, M3-6, Hen2-29 and Hen2-37
covering the spectral range, 3400-7000 A. We derive the ionisation structure,
the physical conditions, the chemical compositions and the kinematical
characteristics of these PNe and find good agreement with previous studies that
relied upon the long-slit technique in their co-spatial area. From their
chemical compositions as well as their spatial and kinematic characteristics,
we determined that Hen2-29 is of the Peimbert Type I (He and N rich), while the
other three are of Type II. The strength of the nebular He II line reveals that
M3-3, Hen2-29 and Hen2-37 are of mid to high excitation classes while M3-6 is a
low excitation planetary nebula (PN). A series of emission-line maps extracted
from the data cubes were constructed for each PN to describe its overall
structure. These show remarkable morphological diversity. Spatially resolved
spectroscopy of M3-6, shows that the recombination lines of CII, CIII, CIV and
NIII are of nebular origin, rather than arising from the central star as had
been previously proposed. This result increases doubts regarding the weak
emission-line star (WELS) classification raised by Basurah et al. (2016). In
addition, they reinforce the probability that most genuine cases of WELS are
arise from irradiation effects in close binary central stars (Miszalski 2009).
