A comparative study of radio signatures from winds and jets: modelling synchrotron emission and polarization
ABSTRACT Outflows driven by active galactic nuclei (AGNs) are seen in numerous compact sources; however, it has remained unclear how to distinguish between the driving mechanisms, such as winds and jets. Therefore, our study aims to offer observational insights from simulations to aid in this distin...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2024-09, Vol.533 (2), p.2213-2231 |
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Sprache: | eng |
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