Star formation is inefficient. Only a few per cent of the available gas in molecular clouds
forms stars, leading to the observed low star formation rate (SFR). The same holds when …

We combine previously published interferometric and single-dish data of relatively nearby
massive dense cores that are actively forming stars to test whether their 'fragmentation …

We investigate the interplay between magnetic (B) field, gravity, and turbulence in the
fragmentation process of cores within the filamentary infrared dark cloud G34. 43+ 00.24 …

Context. The Galactic Faraday depth sky is a tracer for both the Galactic magnetic field and
the thermal electron distribution. It was previously reconstructed from polarimetric …

We study the dynamical state of massive cores by using a simple analytical model, an
observational sample, and numerical simulations of collapsing massive cores. From the …

We present magnetohydrodynamic simulations aimed at studying the effect of the magnetic
suppression of turbulence (generated through various instabilities during the formation of …

Angular dispersion functions are typically used to estimate the fluctuations in polarization
angle around the mean magnetic field orientation in dense regions, such as molecular …

We analyze the physical properties and energy balance of density enhancements in two
SPH simulations of the formation, evolution, and collapse of giant molecular clouds. In the …

We present radiation-magnetohydrodynamic simulations aimed at studying evolutionary
properties of H ii regions in turbulent, magnetized, and collapsing molecular clouds formed …

We apply correlation analysis to random fields in numerical simulations of the supernova-
driven interstellar medium (ISM) with the magnetic field produced by dynamo action. We …