  We have considered the existence of neutron star magnetic field given by the
cyclotron lines. We collected the data of 9 sources of high-mass X-ray binaries
with supergiant companions as a case of testing our model, to demonstrate their
distribution and evolution. The wind velocity, spin period and magnetic field
strength are studied under different mass loss rate. In our model, correlations
between mass-loss rate and wind velocity are found and can be tested in further
observations. We examined the parameter space where wind accretion is allowed,
avoiding barrier of rotating magnetic fields, with robust data of magnetic
field of neutron stars. Our model shows that most of sources (6 of 9 systems)
can be fed by the wind with relatively slow velocity, and this result is
consistent with previous predictions. In a few sources, our model cannot fit
under the standard wind accretion scenario. In these peculiar cases, other
scenarios (disk formation, partial Roche lobe overflow) should be considered.
This would provide information about the evolutionary tracks of various types
of binaries, and thus show a clear dichotomy behavior in wind-fed X-ray binary
systems.
