A Novel Method of Modeling Extended Emission of Compact Jets: Application to Swift J1727.8−1613
Flat radio spectra of compact jets launched by both supermassive and stellar-mass black holes (BHs) are explained by an interplay of self-absorbed synchrotron emission up to some distance along the jet and optically thin synchrotron at larger distances. Their spatial structure is usually studied usi...
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| Principais autores: | , , |
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| 格式: | Artigo |
| 語言: | Inglês |
| 出版: |
IOP Publishing
2025-01-01
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| 叢編: | The Astrophysical Journal Letters |
| 主題: | |
| 在線閱讀: | https://doi.org/10.3847/2041-8213/ade13b |
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