Supermassive black holes in radio-loud AGN
arXiv:astro-ph/0302455 · doi:10.1016/S1387-6473(03)00020-4
Abstract
In this review the correlations between host galaxy properties and black-hole mass determined from nearby quiescent galaxies are briefly discussed, before proceeding to investigate their application to active galactic nuclei (AGN). The recent advances in estimating the black-hole masses of AGN are then reviewed, followed by an examination of the connection between black-hole mass and radio luminosity.
arXiv comment8 pages, 4 figures, To appear in "Radio galaxies: past, present & future". eds. M. Jarvis et al., Leiden, Nov 2002
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