Italian astronomers have developed a 3-D model for the supernova remnant (SNR) IC 443 in order to investigate the morphology of this source. The model allowed the researchers to gain more insights into the complex morphology of SNR IC 443 and provided crucial information about X-ray emission from this object. The study was detailed in a paper published December 15 on arXiv.org.
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Source: Phys.org