  With the Suzaku satellite, we observed an unidentified TeV gamma-ray source
HESS J1741$-$302 and its surroundings. No diffuse or point-like X-ray sources
are detected from the bright southern emission peak of HESS J1741$-$302. From
its neighborhood, we found a new intermediate polar candidate at the position
of $(\alpha, \delta)_{\rm J2000.0} = (\timeform{17h40m35.6s},
\timeform{-30D14m16s})$, which is designated as Suzaku J174035.6$-$301416. The
spectrum of Suzaku J174035.6$-$301416 exhibits emission lines at the energy of
6.4, 6.7 and 7.0 keV, which can be assigned as the K$\alpha$ lines from
neutral, He-like and H-like iron, respectively. A coherent pulsation is found
at a period of 432.1 $\pm$ 0.1 s. The pulse profile is quasi-sinusoidal in the
hard X-ray band (4$-$8 keV), but is more complicated in the soft X-ray band
(1$-$3 keV). The moderate period of pulsation, the energy flux, and the
presence of the iron K$\alpha$ lines indicate that Suzaku J174035.6$-$301416 is
likely an intermediate polar, a subclass of magnetized white dwarf binaries
(cataclysmic variables).
  Based on these discoveries, we give some implications on the origin of GCDX
and brief comments on HESS J1741$-$302 and PSR B1737$-$30.

High Energy Astrophysical Phenomena