Synchrotron Self-absorption Spectral Modeling Reveals a Magnetically Driven Shock-in-jet Scenario in Blazar 1156+295

Unveiling the launching and driving mechanisms of powerful jets in active galactic nuclei is crucial for understanding the coevolution of supermassive black holes and their host galaxies. 1156+295 is a blazar at a redshift of z = 0.729 and exhibits significant variability in long-term radio monitori...

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Auteurs principaux:	Wancheng Xu, Lang Cui, Tao An, Sándor Frey, Xin Wang, Yuanqi Liu, Ning Chang, Liang Chen, Yingkang Zhang
Format:	Artigo
Langue:	Inglês
Publié:	IOP Publishing 2026-01-01
Collection:	The Astrophysical Journal
Sujets:	Blazars Active galactic nuclei Interstellar synchrotron emission Relativistic jets Magnetic fields
Accès en ligne:	https://doi.org/10.3847/1538-4357/ae5529
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