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Core-collapse supernovae as cosmic ray sources
Core-collapse supernovae produce fast shocks which pervade the dense circumstellar medium (CSM) of the stellar progenitor. Cosmic rays (CRs) if accelerated at these shocks can induce the growth of electromagnetic fluctuations in the foreshock medium. In this study, using a self-similar description o...
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| Udgivet i: | Mon Not R Astron Soc |
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| Main Authors: | , , , , |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
2018
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| Fag: | |
| Online adgang: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7735205/ https://ncbi.nlm.nih.gov/pubmed/33324024 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1093/mnras/sty1743 |
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