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From Supernova to Remnant: Tracking the Evolution of the Oldest Known X-Ray Supernovae
Core-collapse supernovae (SNe) expand into a medium created by winds from the pre-SN progenitor. The SN explosion and resulting shock wave(s) heat up the surrounding plasma, giving rise to thermal X-ray emission, which depends on the density of the emitting material. Tracking the variation of the X-...
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| 出版年: | Astrophys J |
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| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
2020
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| 主題: | |
| オンライン･アクセス: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7735324/ https://ncbi.nlm.nih.gov/pubmed/33328690 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/1538-4357/abb087 |
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