3C 397 vs W49B
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3C 397
3C 397, also designated G41.1-0.3, is a supernova remnant in the Milky Way and a radio source listed in the Third Cambridge Catalogue. X-ray observations show unusually high abundances of iron-group elements including iron, nickel, manganese, and chromium. Its asymmetric, clumpy structure and chemical composition are studied as evidence about the Type Ia supernova that produced the remnant.
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W49B
W49B represents the expanding debris field of a long-dead star located in the Aquila constellation approximately 33,000 light-years from Earth. This supernova remnant is particularly interesting due to its irregular shape, suggesting a complex explosion mechanism possibly involving jets. Astronomers study W49B to understand the final stages of massive star evolution and the processes involved in c...
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