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- W1902886916 abstract "Accreting black holes on all mass scales (from stellar to supermassive) appear to follow a nonlinear relation between X-ray luminosity, radio luminosity and BH mass, indicating that similar physical processes drive the central engines in X-ray binaries and active galactic nuclei (AGN). However, in recent years an increasing number of BH systems have been identified that do not fit into this scheme. These outliers may be the key to understand how BH systems are powered by accretion. Here we present results from EVN observations of a sample of low-luminosity AGN (LLAGN) with known mass that have unusually high radio powers when compared with their X-ray luminosity." @default.
- W1902886916 created "2016-06-24" @default.
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- W1902886916 date "2013-03-05" @default.
- W1902886916 modified "2023-10-14" @default.
- W1902886916 title "LLAGN and jet-scaling probed with the EVN" @default.
- W1902886916 cites W2032911527 @default.
- W1902886916 doi "https://doi.org/10.48550/arxiv.1303.1072" @default.
- W1902886916 hasPublicationYear "2013" @default.
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