Turbulence Implies that Mean Motion Resonances are Rare
Authors:
- Fred C. AdamsFAFred C. Adams
- Gregory LaughlinGLGregory Laughlin
- Anthony M. BlochABAnthony M. Bloch
- 20 August 2008
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 683 (2) , 1117-1128
Abstract
No abstract availableKeywords
This publication has 33 references indexed in Scilit:
- Five Planets Orbiting 55 CancriThe Astrophysical Journal, 2008
- Hill's Equation with Random Forcing TermsSIAM Journal on Applied Mathematics, 2008
- Enhanced Cosmic-Ray Flux and Ionization for Star Formation in Molecular Clouds Interacting with Supernova RemnantsThe Astrophysical Journal, 2006
- Catalog of Nearby ExoplanetsThe Astrophysical Journal, 2006
- Planetary migration and extrasolar planets in the 2/1 mean-motion resonanceMonthly Notices of the Royal Astronomical Society, 2005
- Eccentricity Evolution for Planets in Gaseous DisksThe Astrophysical Journal, 2003
- Enhancement of Ambipolar Diffusion Rates through Field FluctuationsThe Astrophysical Journal, 2002
- Layered Accretion in T Tauri DisksThe Astrophysical Journal, 1996
- A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolutionThe Astrophysical Journal, 1991
- Derivation and Application of the Fokker-Planck Equation to Discrete Nonlinear Dynamic Systems Subjected to White Random ExcitationThe Journal of the Acoustical Society of America, 1963