High-resolution simulations of planetesimal formation in turbulent protoplanetary discs

Authors: A. Johansen, H. Klahr and Th. Henning.<br />Astronomy & Astrophysics Vol. 529 , page A62<br />Published online: 01/04/2011<br />
Keywords:
accretion, accretion disks ; methods: numerical ; magnetohydrodynamics (MHD) ; planets and satellites: formation ; planetary systems ; turbulence.

Related Posts

Comments are closed.