July 1999 from the BeppoSAX Calendar
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Intensity plot and (5.9-7.3 keV) X-ray image of Cas A, the youngest
supernova remnant in our galaxy. The regions of high emission apparent in these
images, taken at the beginning of the BeppoSAX mission, during
the Science Verification Phase, are due to spectral lines from the Fe K complex.
Courtesy of M.C. Maccarone, IFCAI/CNR, Palermo, Italy
Images courtesy of the Agenzia Spaziale Italiana (ASI) and the
BeppoSAX Science Data Center (SDC).
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