  We present the result from a CHANDRA observation of an X-ray luminous
starburst galaxy UGC 6697, which is embedded in the northwest hot region of
A1367 (5 - 6 keV). A very sharp X-ray edge (~ 13 times of surface brightness
jump) at the southeast and a long tail (at least 60 kpc from the nucleus) at
the northwest of the galaxy are detected, as expected if the galaxy is moving
to the southeast. The X-ray edge, at the midway of the nucleus and the
southeast optical disk edge, is also at the same position where the Halpha
emission is truncated and a radio sharp edge is observed. The X-ray diffuse
emission is also enhanced at the southeast, implying ram pressure compression.
No extraplanar X-ray component is detected, probably due to the combining
effects of weaker outflow activity than that in nuclear starbursts, and
external confinement plus stripping. The diffuse thermal gas in UGC 6697 has a
temperature of ~ 0.7 keV and a low iron abundance (~0.1 - 0.2 solar). An X-ray
point source (L (0.5-10 keV) ~ 2.8 x 10^{40} ergs s^{-1}) is detected on the
nucleus, but not highly absorbed. Three off-center ultraluminous X-ray sources,
all with L (0.5-10 keV) > 10^{40} ergs s^{-1}, are also detected. Based on the
multi-wavelength data available, we favor that the interaction between the
interstellar medium (ISM) and the ICM plays a major role to trigger the
starburst in UGC 6697.
