Abstract
AbstractWe present a brief review of emission-line velocity differences, and describe an ongoing project to determine the driving mechanisms responsible. We conclude with a brief outline of the use of velocity differences as probes of the conditions in the nuclear region of AGNs.
Publisher
Cambridge University Press (CUP)
Cited by
1 articles.
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1. The Broad-Line Region in Active Galactic Nuclei;Physics of Active Galactic Nuclei at all Scales