Abstract
We present here the results of the mapping observation of the Cygnus Loop with the Gas Imaging Spectrometer (GIS) onboard the ASCA observatory. The data covered the entire region of the Cygnus Loop. Spatial resolution of the GIS is moderate whereas the energy resolving power is much better than those used in the previous observations. The ASCA soft-band image shows the well-known shell-like feature whereas the ASCA hard-band image shows rather center-filled morphology with a hard X-ray compact source at the blow-up southern region.
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