An exact model for magnetized and rotating outflows, underpressured at their axis, is
analysed by means of a nonlinear separation of the variables in the two-dimensional …

Context. It is well established that some YSO jets (eg RW Aur) display different propagation
speeds between their blue and red shifted parts, a feature possibly associated with the …

Ordinary differential equations describing the self-similar collapse of a rotating, magnetized,
self-gravitating and isothermal filament are derived. Explicit homologous solutions are …

Powerful, highly collimated jets, surrounded by bipolar molecular outflows, are commonly
observed near Young Stellar Objects (YSOs). In the usual theoretical picture of star …

Magnetic fields may relax dissipatively to the minimum energy force-free condition whenever
they are not constantly created or distorted. We review the axially symmetric solutions for …

We propose an extension of the semi-analytical solutions derived by Lin et al.([CITE])
describing the two-dimensional homologous collapse of a self-gravitating rotating cloud …

X-ray observations have shown that, like all late-type stars, young, low-mass stars are
magnetized. X-ray flaring characteristics suggest that the resulting activity is solar-like, with X …

The long lasting lack of understanding of star formation is mainly due to the fact that the
process has never been directly observed. Indeed, stars begin their lives deep inside dense …

It is a well established fact that some YSO jets (eg RW Aur) display different propagation
speeds between their blue and red shifted parts, a feature possibly associated with the …

Context. It is a well established fact that some YSO jets (eg RW Aur) display different
propagation speeds between their blue and red shifted parts, a feature possibly associated …