Summary
Active Galactic Nuclei Jets (AGN) are complex astrophysics phenomena. Understanding their mechanism involve many aspect of the theory of high energy physics (general relativity, fluid mechanics, radiative physics, electro-magnetism, relativistic thermodynamics…). There is a need to build pertinent models of these flows to explain the main involved physical mechanisms, to make numerical simulations and study their role in the formation and the history of galaxies. There is also a lot of work to observe these such distant phenomena with the goal of getting the most pertinent explanation.
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Chantry, L.,Cayatte, V.,Sauty, C.,Vlahakis, N.,Tsinganos, K.. A&A, 612:A63, April 2018
Globus, N.,Levinson, A.. PRd, 88(8):084046, October 2013.
Meliani, Z.,Sauty, C.,Vlahakis, N.,Tsinganos, K.,Trussoni, E.. A&A, 447:797–812, March 2006.
Sauty, C.,Tsinganos, K., A&A, 287:893–926, July 1994.
M. Zamaninasab, E. Clausen-Brown, T. Savolainen, and A. Tchekhovskoy. Nature, 510:126–128, June 2014
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Chantry, L. (2019). Meridional Self-Similar MHD Relativistic Flows Around Kerr Black Holes. In: Sauty, C. (eds) JET Simulations, Experiments, and Theory. Astrophysics and Space Science Proceedings, vol 55. Springer, Cham. https://doi.org/10.1007/978-3-030-14128-8_3
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DOI: https://doi.org/10.1007/978-3-030-14128-8_3
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