364 citations · 2.2k across the 40 of their papers we have counts for
40 papers
Numerical simulations of MHD jets from Keplerian accretion disks I-Recollimation shocks
Thomas Jannaud, Claudio Zanni, Jonathan Ferreira
Aims. We wish to establish a firm link between jet simulations and analytical studies of magnetically-driven steady-state jets from Keplerian accretion disks. In particular, the la…
Absorption lines from magnetically driven winds in X-ray binaries II: high resolution observational signatures expected from future X-ray observatories
Susmita Chakravorty, Pierre-Olivier Petrucci, Sudeb Ranjan Datta +12
In our self-similar, analytical, magneto-hydrodynamic (MHD) accretion-ejection solution, the density at the base of the outflow is explicitly dependent on the disk accretion rate -…
Are Low-Frequency Quasi-Periodic Oscillations seen in accretion flows the disk response to a jet instability?
Jonathan Ferreira, Gregoire Marcel, Pierre-Olivier Petrucci +7
Low Frequency Quasi-Periodic Oscillations or LF QPOs are ubiquitous in BH X-ray binaries and provide strong constraints on the accretion-ejection processes. Although several models…
First Detection of Interaction between a Magnetic Disk Wind and an Episodic Jet in a Protostellar System
Chin-Fei Lee, Benoit Tabone, Sylvie Cabrit +6
Rotating outflows from protostellar disks might trace extended magneto-hydrodynamic (MHD) disk winds (DWs), providing a solution to the angular momentum problem in disk accretion f…
Magnetic outflows from turbulent accretion disks: I. Vertical structure & secular evolution
J. Jacquemin-Ide, G. Lesur, J. Ferreira
Astrophysical disks are likely embedded in an ambient vertical magnetic field. This ambient field is known to drive magneto-rotational turbulence in the disk bulk but is also respo…
Jets from Young Stars
T. P. Ray, J. Ferreira
Jets are ubiquitous in the Universe and, as demonstrated in this volume, are seen from a large number of astrophysical objects. For a number of reasons, in particular their proximi…