On the Azimuthal Structure of Thermal Convection in Circumstellar Disks
- 20 March 1999
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 514 (1) , 325-343
- https://doi.org/10.1086/306926
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- The Piecewise Parabolic Method (PPM) for gas-dynamical simulationsPublished by Elsevier ,2004
- Particle-Trapping Eddies in Protoplanetary Accretion DisksIcarus, 1997
- Numerical Simulations of Circumstellar Disk ConvectionThe Astrophysical Journal, 1996
- Using FU Orionis outbursts to constrain self-regulated protostellar disk modelsThe Astrophysical Journal, 1994
- Large Eddy simulation of turbulence: A subgrid scale model including shear, vorticity, rotation, and buoyancyThe Astrophysical Journal, 1994
- On the Angular Momentum Transport Associated with Convective Eddies in Accretion DisksThe Astrophysical Journal, 1993
- Planet FormationAnnual Review of Astronomy and Astrophysics, 1993
- A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolutionThe Astrophysical Journal, 1991
- A flux-limited diffusion theoryThe Astrophysical Journal, 1981
- Physics of the primitive solar accretion diskEarth, Moon, and Planets, 1978