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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Bibliographic Details
Published in:	The Astrophysical Journal Letters
Main Authors:	Andrzej A. Zdziarski, Callan M. Wood, Francesco Carotenuto
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Subjects:	Low-mass x-ray binary stars Radio jets Relativistic jets X-ray transient sources
Online Access:	https://doi.org/10.3847/2041-8213/ade13b

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