  We investigate the galactic axes orientations within 18 selected clusters,
sub-structures of the Local Supercluster. For every cluster we map the
parameter \Delta_{11} (Flin & God{\l}owski 1986) describing the galactic axes
alignment with respect to a cluster pole changing along the entire celestial
sphere. The resulting maps are analyzed for correlations of its maxima with
directions from the cluster centre to 1.) the derived `physical' cluster poles,
2.) the Local Supercluster centre, 3.) the Virgo A centre and 4.) the Earth,
i.e. along the line of sight (LOS). The strong maxima - with one exception -
exist only for non-spiral (NS) sub-samples, with the maximum well correlated
with the LOS direction. For clusters with a clearly defined weak maximum the
conclusion generally does not change. For the spiral (S) sub-samples the maps
are usually at the random noise level. In these cases a weaker, but still
existent correlation with the LOS is observed and no other evident correlations
are noted. We conclude that the strong systematic effect, generated by the
process of galactic axis de-projection from its optical image, is present in
the catalogue data. With the use of a simple model for the systematic effect we
are able to reproduce the main characteristic features of the maps for NS
galaxies. We note, however, a few clusters showing significant differences with
respect to this model.
