EHT data show a 51.8 microarcsecond ring around Sgr A* consistent with the shadow of a 4 million solar mass Kerr black hole viewed at moderate inclination.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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Proposes a diagnostic framework using scale-dependent spectral properties from SSA and FFA to distinguish jets, coronae, outflows, and star formation in RQ AGN for SKA multi-frequency imaging.
citing papers explorer
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Probing the Parsec-Scale Dynamical Structure of Ionized Gas in Radio-Quiet AGN with SKA
Proposes a diagnostic framework using scale-dependent spectral properties from SSA and FFA to distinguish jets, coronae, outflows, and star formation in RQ AGN for SKA multi-frequency imaging.