BeppoSAX Observations of the Galactic Center Region: Soft x-rays from the radio halo of SgrAEast

Abstract

The BeppoSAX satellite performed a survey of the Galactic Center Region in the 1-10 keV energy band with its Narrow Field Instruments. Several bright X-ray sources containing neutron stars and black holes have been observed and studied, including the possible counterpart of SgrA*. Here we report the results on the diffuse emission coming from the SgrA Complex. The emission from within 8 arcmin from SgrA* has a double-temperature thermal spectrum (kT1~0.6 keV and kT2~8 keV) and an energy-dependent morphology: the hard emission (5-10 keV) is elongated along the galactic plane, while the soft one (2-5 keV) shows a triangular shape, very similar to the radio halo of SgrAEast. This spatial correlation and the physical parameters of the lower temperature component support the interpretation of the radio halo of the Sgr~A~East shell as a SNR.