  We report on new VLA radio and XMM-Newton X-ray observations of the SNR
G352.7-0.1. These high sensitivity, high resolution data reveal that G352.7-0.1
belongs to the thermal composite morphological class. Small scale structures in
radio and X-ray emission are not always correlated and are different for the
different X-rays bands examined. The distance to G352.7-0.1 can be constrained
between 6.6 and 8.4 kpc. The study of the HI suggests that G352.7-0.1 is
located within a cavity probably created by the stellar wind of the precursor
star.
