  We present the results of our morphological and spectral study of properties
of the supernova remnant RX J1713.7-3946 based on data obtained with
XMM-Newton. Highly inhomogeneous structures, such as the bright spots,
filaments and dark voids, noted by Uchiyama et al. (2003), appear in the entire
bright western portion of the shell. In addition two narrow rims are found
which run parallel to each other from north to south in the western part of the
remnant. No complex structures are seen in the interior region of the remnant.
The X-ray spectra everywhere can be well represented with a power-law function
of photon index ranging within Gamma = 2.0-2.8. A clear difference of spectra
between the central dim region and the bright western portion is seen at lower
energies. This differences can be ascribed either to an additional thermal
component with electron temperature, kTe= 0.56keV from the center or,
alternatively, to an increase in column density of Delta NH ~ 0.3 x 10^22 cm^-2
in the western region. In the context of the recent discovery by the NANTEN
telescope of a molecular cloud apparently interacting with the western part of
the supernova remnant, the second possibility seems to be the more likely
scenario.

Astrophysics