Related references
Note: Only part of the references are listed.Clumps in the outer disk by disk instability: Why they are initially gas giants and the legacy of disruption
Aaron C. Boley et al.
ICARUS (2010)
Introducing a hybrid radiative transfer method for smoothed particle hydrodynamics
Duncan Forgan et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
Pseudo-viscous modelling of self-gravitating discs and the formation of low mass ratio binaries
C. J. Clarke
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
The properties of brown dwarfs and low-mass hydrogen-burning stars formed by disc fragmentation
Dimitris Stamatellos et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2009)
Can giant planets form by gravitational fragmentation of discs?: Radiative hydrodynamic simulations of the inner disc region (≲40 AU)
D. Stamatellos et al.
ASTRONOMY & ASTROPHYSICS (2008)
The formation of fragments at corotation in isothermal protoplanetary disks
Richard H. Durisen et al.
ASTROPHYSICS AND SPACE SCIENCE (2008)
Numerical requirements for simulations of self-gravitating and non-self-gravitating discs
Andrew F. Nelson
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2006)
Investigating fragmentation conditions in self-gravitating accretion discs
WKM Rice et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2005)
The effect of cooling on the global stability of self-gravitating protoplanetary discs
WKM Rice et al.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2003)
Formation of giant planets by fragmentation of protoplanetary disks
L Mayer et al.
SCIENCE (2002)
Share Paper
