Turning AGN Bubbles into Radio Relics with Sloshing: Modeling CR Transport with Realistic Physics
Radio relics are arc-like synchrotron sources at the periphery of galaxy clusters, produced by cosmic-ray electrons in a <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mi mathvariant="sans-serif">μ</mi></semantics></math></inline-formula>G magnetic fiel...
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| Materialtyp: | Artigo |
| Språk: | Inglês |
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MDPI AG
2021-11-01
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| Serie: | Galaxies |
| Ämnen: | |
| Länkar: | https://www.mdpi.com/2075-4434/9/4/91 |
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