In this chapter I will review the status of our phenomenological understanding of the relation between accretion and outflows in accreting black hole systems. This understanding arises primarily from observing the relation between X-ray and longer wavelength (infrared, radio) emission. The view is necessarily a biased one, beginning with observations of X-ray binary systems, and attempting to see if they match with the general observational properties of active galactic nuclei. © 2010 Springer-Verlag Berlin Heidelberg.
CITATION STYLE
Fender, R. (2009). “Disc-jet” coupling in black hole x-ray binaries and active galactic nuclei. Lecture Notes in Physics, 794, 115–142. https://doi.org/10.1007/978-3-540-76937-8_5
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