A comparative study of disc-planet interaction
Top Cited Papers
Open Access
- 22 June 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 370 (2) , 529-558
- https://doi.org/10.1111/j.1365-2966.2006.10488.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 53 references indexed in Scilit:
- The Piecewise Parabolic Method (PPM) for gas-dynamical simulationsPublished by Elsevier ,2004
- Orbital Migration and Mass Accretion of Protoplanets in Three‐dimensional Global Computations with Nested GridsThe Astrophysical Journal, 2003
- Hydromagnetic turbulence in computer simulationsComputer Physics Communications, 2002
- Gas Giant Protoplanet Formation: Disk Instability Models with Thermodynamics and Radiative TransferThe Astrophysical Journal, 2001
- Tidally Induced Gap Formation in Protostellar Disks: Gap Clearing and Suppression of Protoplanetary GrowthThe Astrophysical Journal, 1999
- Evolution of the Solar Nebula. IV. Giant Gaseous Protoplanet FormationThe Astrophysical Journal, 1998
- Modelling accretion in protobinary systemsMonthly Notices of the Royal Astronomical Society, 1995
- von Neumann stability analysis of smoothed particle hydrodynamics—suggestions for optimal algorithmsJournal of Computational Physics, 1995
- Higher order Godunov schemes for isothermal hydrodynamicsThe Astrophysical Journal, 1994
- The piecewise-parabolic method in curvilinear coordinatesThe Astrophysical Journal Supplement Series, 1993