We present the first results of astrophysically relevant experiments where highly supersonic
plasma jets are generated via conically convergent flows. The convergent flows are created …

The dynamics of plasma and neutral gas in pressure balance are solved self-consistently to
reveal the impact of neutral depletion. Analytical relations that determine the electron …

Highly collimated supersonic jets and less collimated outflows are observed to emerge from
a wide variety of astrophysical objects. They are seen in young stellar objects (YSOs), proto …

Protostellar jets most probably originate in turbulent accretion disks surrounding young
stellar objects. We investigate the evolution of a disk wind into a collimated jet under the …

Although several lines of evidence suggest that jets from young stars are driven
magnetically from accretion disks, existing observations of field strengths in the bow shocks …

Context. The young stellar object (YSO) Th 28 possesses a highly collimated jet, which
clearly exhibits an asymmetric brightness of its jet lobes at optical and near-infrared …

Context. Interstellar magnetic fields influence all stages of the process of star formation, from
the collapse of molecular cloud cores to the formation and evolution of circumstellar disks …

We present the results of a series of axisymmetric time-dependent magnetohydrodynamic
(MHD) simulations of the propagation of cooling, overdense jets. Our numerical models are …

We study the Hα emission from jets using two-dimensional axisymmetrical simulations. We
compare the emission obtained from hydrodynamic (HD) simulations with that obtained from …

We here investigate, by means of fully three-dimensional smoothed particle
magnetohydrodynamic numerical simulations, the effects of different initial magnetic field …