Researchers from Harvard-Smithsonian Center for Astrophysics (CfA) have conducted detailed spectroscopy of N132D—an X-ray bright supernova remnant (SNR) in the Large Magellanic Cloud (LMC). Results of the study, presented in a paper published April 15 on the arXiv pre-print server, provide important information about the chemical composition of this SNR and shed more light on its origin.
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Source: Phys.org