A Study of 3C 397, a Supernova Remnant (IMAGE)
Caption
This is a study of 3C 397, a supernova remnant shown here in X-rays from NASA's Chandra X-ray Observatory (purple) and Suzaku (blue), indicates the blast arose from a single white dwarf that accumulated matter from a normal companion star. The white dwarf exploded as its mass neared 1.4 solar masses.
Credit
NASA/Suzaku and NASA/CXC, DSS, and NASA/JPL-Caltech
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