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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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Bibliografiset tiedot
Päätekijät: Andrzej A. Zdziarski, Callan M. Wood, Francesco Carotenuto
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2025-01-01
Sarja:The Astrophysical Journal Letters
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Linkit:https://doi.org/10.3847/2041-8213/ade13b
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