We describe the algorithms implemented in the first version of GRADSPH, a parallel, tree-
based, smoothed particle hydrodynamics code for simulating self-gravitating astrophysical …

The collapse and fragmentation of molecular cloud cores is examined numerically with
unprecedentedly high spatial resolutions, using the publicly released code GADGET-2. As …

The growing observational evidence that main-sequence and pre-main-sequence protostars
are found in binary and multiple systems suggests that they are formed by a fragmentation of …

The continued detection of binary systems among pre-main-sequence stars suggests that
fragmentation is a very frequent process during the early stages of star formation. However …

Observations in X-ray and EUV of the solar corona reveal the existence of very complex and
dynamic structures made of plasma magnetically confined in loops. These structures can be …

In this paper we present the results of a set of numerical simulations aimed to study the
gravitational collapse of a spherically symmetric, rigidly rotating, isolated, interstellar gas …

We consider 28 particle-based simulations aimed at comparing the gravitational collapse of
a spherically symmetric, uniform gas core in which two extreme types of turbulent spectra of …

We present a set of numerical simulations of the gravitational collapse of a uniform and
rotating core, in which azimuthal symmetric mass seeds are initially implemented in order to …

En este trabajo estudiamos el colapso gravitacional de una nube de gas de hidrógeno
molecular compuesta de un núcleo más una envolvente de gas rodeando al núcleo …

We present high-resolution hydrodynamical simulations aimed at following the gravitational
collapse of a gas core, in which a turbulent spectrum of velocity is implemented only initially …