In many ways the discovery that star formation involves outflow as well as inflow from
gravitational collapse marked the beginning of modern studies of the assembly of stars. Jets …

Powerful relativistic jets are one of the main ways in which accreting black holes provide
kinetic feedback to their surroundings. Jets launched from or redirected by the accretion flow …

Powerful jets and outflows are launched from the protostellar disks around newborn stars.
These outflows carry enough mass and momentum to transform the structure of their parent …

Disk–Jet Coupling in the 2017/2018 Outburst of the Galactic Black Hole Candidate X-Ray
Binary MAXI J1535–571 - IOPscience This site uses cookies. By continuing to use this site you …

We wish to constrain the possible contribution of a magnetohydrodynamic disk wind (DW) to
the HH212 molecular jet. We mapped the flow base with ALMA Cycle 4 at 0. ̋13~ 60 au …

The surroundings of massive protostars constitute an accretion disc which has numerically
been shown to be subject to fragmentation and responsible for luminous accretion-driven …

Aims. High-resolution Very-Long-Baseline Interferometry (VLBI) observations of relativistic
jets are essential for constraining the fundamental parameters of jet formation models. At a …

We perform a series of three-dimensional, magnetohydrodynamical simulations of star
cluster formation including gravity, turbulence, magnetic fields, stellar radiative heating, and …

The formation and evolution of a wide class of astrophysical objects are governed by
turbulent, magnetized accretion disks. Understanding their secular dynamics is of primary …

Turbulence is a critical ingredient for star formation, yet its role for the initial mass function
(IMF) is not fully understood. Here we perform magnetohydrodynamical (MHD) simulations …