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From Protoplanetary Disks to Circumplanetary Disks
The numerical code PHYVE is a hydrodynamical code that allows to follow the formation and evolution of protoplanetary disks from the collapse of the molecular cloud to the photoevaporation phase. This code is able to model the surface mass density distribution consistently with the disk radial profile (including the disk composition and geometry).openaire +1 more source
Gravitational Instabilities in Circumstellar Disks
Annual Review of Astronomy and Astrophysics, 2016Kaitlin M Kratter, Giuseppe Lodato
exaly

