Simulating radially outward winds within a turbulent gas clump
  By using the particle-based code Gadget2, we follow the evolution of a gas
clump, in which a gravitational collapse is initially induced. The particles
representing the gas clump have initially a velocity according to a turbulent
spectrum built in a Fourier space of 64$^3$ grid elements. In a very early
stage of evolution of the clump, a set of gas particles representing the wind,
suddenly move outwards from the clump's center. We consider only two kinds of
winds, namely: one with spherical symmetry and a second one being a bipolar
collimated jet. In order to assess the dynamical change in the clump due to
interaction with the winds, we show iso-velocity and iso-density plots for all
our simulations.
