  The binding energies of neutron rich strangeness $S=-1$ hypernuclei are
estimated in the chiral soliton approach using the bound state rigid oscillator
version of the SU(3) quantization model. Additional binding of strange
hypernuclei in comparison with nonstrange neutron rich nuclei takes place at
not large values of atomic (baryon) numbers, $A=B\leq\sim 10$. This effect
becomes stronger with increasing isospin of nuclides, and for "nuclear variant"
of the model with rescaled Skyrme constant $e$. Total binding energies of
(Lambda)He-8 and recently discovered (Lambda)H-6 satisfactorily agree with
experimental data. Hypernuclei (Lambda)H-7, (Lambda)He-9 are predicted to be
bound stronger in comparison with their nonstrange analogues H-7, He-9;
hypernuclei (Lambda)Li-10, (Lambda)Li-11, (Lambda)Be-12, (Lambda)Be-13, etc.
are bound stronger in the nuclear variant of the model.
