Summary
Recent magnetohydrodynamic (MHD) simulations are presented investigating the launching of jets from accretion disks, that is (i) the internal disk structural evolution that leads to different launching conditions over time, (ii) a new, fundamental interrelation between the disk magnetization at the launching point and the asymptotic outflow properties, (iii) the launching of jets driven by a self-generated disk dynamo magnetic field, and (iv) simulations of jets from orbiting jet sources.
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Acknowledgements
The work discussed above has mostly be done by my students Somayeh Sheiknezami, Bhargav Vaidya, Oliver Porth, Deniss Stepanovs, and Dennis Gaßmann. I thank them for a fruitful collaboration. For the numerical work we applied the PLUTO code [14]. I thank Andrea Mignone and the PLUTO team for the possibility of using their code.
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Fendt, C. (2019). Modeling Jet Launching from Accretion Disks. 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_10
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DOI: https://doi.org/10.1007/978-3-030-14128-8_10
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