Abstract
At present, it is believed that all or most galaxies harbor a massive or even supermassive black hole in their nuclei. Sometimes gas finds its way close to and finally into the black hole. This process of accretion is thought to give rise to an active galactic nucleus and in extreme cases, a quasar. The most widely considered model then involves a black hole, an accretion disk, an obscuring torus (for unification), and, for radio-loud sources, very powerful relativistic radio jets.
Contributions by Mauro D’Onofrio, Paola Marziani, Jack W. Sulentic, Julian Krolik, Martin Gaskell, Suzi Collin, Hagai Netzer, Bozena Czerny, Krzysztof Hryniewicz, Luigi Foschini, Michael Eracleous, Daniel Proga, Paolo Padovani, Serguei Komissarov, Isaac Shlosman, and Martin Elvis
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Notes
- 1.
Anne-Marie Dumont has nothing to do with Simone Dumont with whom the previous papers were written.
- 2.
Another paradigm, presently challenged
- 3.
How the jet is triggered is one of the main unknown of the modern astrophysics.
- 4.
This suggests that the relativistic AGN jets do not originate directly from accretion disks but from their central black holes.
- 5.
I myself wondered back in late 1990s if the orientation of the disk spin could be behind the radio-loud and radio-quiet division and even discussed this idea with Sam Falle, Roger Blandford, and few other colleagues. However, I did not have any clear mechanism in mind. Moreover, the analysis of [338] indicated that retrograde disks were unstable. Finally, the black hole spin paradigm seemed to be a good alternative. In the end, I gave up on this idea. Later, [202] pointed to a flaw in the analysis by [338] and found that prograde disks were in fact stable.
- 6.
I am not sure who exactly proposed this paradigm in the first place. This could have been Chris Reynolds indeed, as the question suggests, but as far as I know, in the scientific literature, this idea first floated in [140].
- 7.
Accretion is growth by gravitational attraction of matter.
- 8.
The proposed mechanism is essentially nonviscous but can be defined in terms of effective viscosity.
- 9.
Spontaneous and induced bars can be accompanied by m = 1, 2, and 3 spiral perturbations.
- 10.
For simplicity, I will use “quasar” for all forms activity associated with a supermassive black hole at the center of a galaxy. In the research literature, no single term spans this range, though “active galactic nuclei” comes close, with “quasar” being reserved for objects above an arbitrary luminosity threshold. To me, this is not a useful division, and “quasar” is a short, memorable, term that serves well.
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D’Onofrio, M. et al. (2012). Models of Quasars. In: D'Onofrio, M., Marziani, P., Sulentic, J. (eds) Fifty Years of Quasars. Astrophysics and Space Science Library, vol 386. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27564-7_6
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