  In continuation of the program formulated in Paper I we present results of
long-slit spectroscopy with the Russian 6m telescope of five more objects from
the Vorontsov-Velyaminov Atlas and Catalogue of Interacting galaxies. These are
the galaxies for which the interaction is not evident, although all of them are
classified as multiple systems (usually as ``nests'', ``chains'' and similar
systems). The spectrophotometry data enable us to derive for all galaxies
abundances of O, and for some of them abundances of N, Ne and S. For two of
them chemical abundances are given for the first time. In spectra of three of
the studied galaxies [Oiii]4363 line is measured, and T_e and oxygen abundance
are derived by the classical method. For the two others, empirical methods are
used. For all 5 galaxies, the radial velocity distribution along the slit was
obtained in the Ha-line. The studied galaxies represent a rather mixed sample:
from very low luminosity irregular galaxies, like VV 499 (DDO 053), to rather
bright VV 523 (NGC 3991). Their metallicities vary from Z=1/25 Zo for VV 499 to
1/2 Zo for VV 523. The morphology of these galaxies ranges between typical dIrr
(VV 080) through ring-like (VV 131) to clumpy Irr (VV 523). Position--Velocity
diagrams in the Ha-line along the galaxy body imply the existence of
large-scale ionized gas outflows/supershells around the sites of intense
current and/or recent SF activity. Sizes of supershells vary in the range of
several hundred pc to about 2 kpc. For all studied galaxies we examine their
local environment and indicate the nearest neighbouring objects capable of
inducing the observed enhanced star formation.
