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Published in 2025 at "Universe"
DOI: 10.3390/universe11060188
Abstract: X-ray emission from supernovae can arise from multiple interactions during their evolution. The immediate explosion is sufficiently energetic to generate X-rays; so, too, is the impact of the shock as it runs into circumstellar matter…
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Keywords:
supernovae;
supernovae chandra;
xmm newton;
chandra xmm ... See more keywords