3D AMR simulations of the evolution of the diffuse gas cloud G2 in the
  Galactic Centre
  With the help of 3D AMR hydrodynamical simulations we aim at understanding
G2's nature, recent evolution and fate in the coming years. By exploring the
possible parameter space of the diffuse cloud scenario, we find that a starting
point within the disc of young stars is favoured by the observations, which may
hint at G2 being the result of stellar wind interactions.
