Exploring the Jet Formation in binary systems applying 3D MHD simulations

We investigate the formation of an ideal magnetized jet that originates from a disk acting as a boundary by conducting axisymmetric MHD simulations. Our simulations demonstrate that the magnetized jet is consistently launched and reaches a stable state. We extended the model setup to three dimension...

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Veröffentlicht in:	arXiv.org 2024-03
Hauptverfasser:	Sheikhnezami, Somayeh, Sepahvand, Mostafa
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion disks Binary systems Companion stars Simulation Tidal effects
Online-Zugang:	Volltext
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