  We present the results of the identification of six objects from the ASCA
Galactic center and Galactic plane surveys: AXJ173548-3207, AXJ173628-3141,
AXJ1739.5-2910, AXJ1740.4-2856, AXJ1740.5-2937, AXJ1743.9-2846. Chandra,
XMM-Newton, and XRT/Swift X-ray data have been used to improve the positions of
the optical counterparts to these sources. Thereafter, we have carried out a
series of spectroscopic observations of the established optical counterparts at
the RTT-150 telescope. Analysis of X-ray and optical spectra as well as
photometric measurements in a wide wavelength range based on optical and
infrared catalogs has allowed the nature of the program sources to be
determined. Two X-ray objects have been detected in the error circle of
AXJ173628-3141: one is a coronally active G star and the other may be a
symbiotic star, a red giant with an accreting white dwarf. Three sources
(AXJ1739.5-2910, AXJ1740.5-2937, AXJ1743.9-2846) have turned out to be active
G-K stars, presumably RS CVn objects, one (AXJ1740.4-2856) is an M dwarf, and
another one (AXJ173548-3207) may be a low-mass X-ray binary in its low state.
The distances and corresponding luminosities of the sources in the soft X-ray
band have been estimated; analysis of deep INTEGRAL Galactic Center
observations has not revealed a statistically significant flux at energies
higher 20 keV from any of them.
