480 citations · 2.4k across the 72 of their papers we have counts for
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MHD simulations of the long-term evolution of a dipolar magnetosphere surrounded by an accretion disk
Ch. Fendt
The evolution of an initially stellar dipole type magnetosphere interacting with an accretion disk is investigated using numerical ideal MHD simulations. The simulations follow sev…
Protostellar jets and magnetic diffusion
M. Cemeljic, Ch. Fendt
We investigate the evolution of a disk wind into a collimated jet under the influence of magnetic diffusivity. Using the ZEUS-3D code in the axisymmetry option we solve the time-de…
Stationary models of relativistic magnetohydrodynamic jets
Christian Fendt
Highly relativistic jets are most probably driven by strong magnetic fields and are launched from the accretion disk surrounding a central black hole. In this paper we review some…
Relativistic MHD jets and the GRBs
Christian Fendt
High velocity highly collimated beams of plasma -- the jets -- are known as a general phenomenon among astrophysical sources of different energy and spatial scale. The common MHD s…
Formation of protostellar jets - effects of magnetic diffusion
Christian Fendt, Miljenko Cemeljic
We investigate the evolution of a disk wind into a collimated jet under the influence of magnetic diffusivity, assuming that the turbulent pattern in the disk will also enter the d…
Theoretical thermal X-ray spectra of relativistic MHD jets
Elisabetta Memola, Christian Fendt, Wolfgang Brinkmann
Highly relativistic jets are most probably driven by strong magnetic fields and launched from the accretion disk surrounding a central black hole. Applying the jet flow parameters…