- Splinter Computation   (virtual room B)

N-Body simulations of the final contraction phase during gravoturbulent formation of planetesimals

Francesco Biscani, Hubert Klahr

Planetesimals can efficiently be formed from the gravitational collapse of pebble clouds. In the past only the concentration and collapse up to Hill density was studied. Here we show the first simulations of the final collapse phase from Hill density to a solid object.