Abstract A model for extragalactic jets considered as magnetized current-carrying structures is presented. The return currents are assumed to flow within the jet itself. Standard MHD equations in cylindrical geometry are used to investigate the equilibrium and stability properties of the model, including the incompressible thermal matter flows in the equilibrium analysis. Absolute stability regions are found and their boundaries are determined. Linear growth rates for the unstable m = 0 and m = 1 modes are computed.

Extragalactic jets as current-carrying systems. I - Equilibrium and stability / Claudio Chiuderi; Paola Pietrini; Guidetta Torricelli Ciamponi. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - STAMPA. - 339:(1989), pp. 70-77. [10.1086/167276]

Extragalactic jets as current-carrying systems. I - Equilibrium and stability

PIETRINI, PAOLA;
1989

Abstract

Abstract A model for extragalactic jets considered as magnetized current-carrying structures is presented. The return currents are assumed to flow within the jet itself. Standard MHD equations in cylindrical geometry are used to investigate the equilibrium and stability properties of the model, including the incompressible thermal matter flows in the equilibrium analysis. Absolute stability regions are found and their boundaries are determined. Linear growth rates for the unstable m = 0 and m = 1 modes are computed.
1989
339
70
77
Claudio Chiuderi; Paola Pietrini; Guidetta Torricelli Ciamponi
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Utilizza questo identificatore per citare o creare un link a questa risorsa: https://hdl.handle.net/2158/776960
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