Asymmetric Jet launching
Aleksandra Kotek, Miljenko \v{C}emelji\'c, W{\l}odek Klu\'zniak and, Deepika A. Bollimpalli

TL;DR
This paper uses resistive and viscous MHD simulations to demonstrate the formation of asymmetric axial jets from star-disk systems, comparing their properties with observations.
Contribution
It introduces the phenomenon of continuous asymmetric jet launching in MHD simulations and analyzes their dynamics and observational relevance.
Findings
Asymmetric jets are launched in certain parameter regimes.
Jets exhibit different speeds and rotation properties.
Simulation results align with recent observational data.
Abstract
In resistive and viscous magnetohydrodynamical (MHD) simulations we obtain axial jets launched from the innermost magnetosphere of a star-disk system. We found that in a part of the parameter space continuous asymmetric jets, which are propagating in opposite directions, are launched. We compare the speed of propagation and rotation of obtained jets with recent observational results.
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Taxonomy
TopicsAstro and Planetary Science · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics
