  Significant fraction of barred galaxies hosts secondary bar-like structures
on optical and NIR images. The circumnuclear dynamics of double-barred objects
are still not well understood, observational data concerning kinematics are
incomplete and inconsistent. In order to compare the simulations results with
observations, we have started new spectroscopic studying of stellar kinematics
in lenticular galaxies from Peter Erwin's catalog of secondary bars. We present
first results concerning their stellar kinematics based on the observations
performed with the integral-field spectrograph MPFS at the Russian 6-m
telescope.
