Sunyaev-Zeldovich signatures from non-thermal, relativistic electrons using CMB maps
Relativistically energetic, non-thermal population of electrons can give rise to unique CMB spectral distortion signatures which can be significantly different from thermal Sunyaev-Zeldovich signal or $y$-distortion. These signatures depend upon the spectrum of non-thermal electrons, therefore, a de...
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| Hlavní autor: | |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
Maynooth Academic Publishing
2024-07-01
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| Edice: | The Open Journal of Astrophysics |
| On-line přístup: | https://doi.org/10.33232/001c.120979 |
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