Phase separation in giant planets: inhomogeneous evolution of Saturn
- 31 July 2003
- Vol. 164 (1) , 228-243
- https://doi.org/10.1016/s0019-1035(03)00130-1
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This publication has 34 references indexed in Scilit:
- The theory of brown dwarfs and extrasolar giant planetsReviews of Modern Physics, 2001
- The [ITAL]Forbidden[/ITAL] Abundance of Oxygen in the SunThe Astrophysical Journal, 2001
- Electrical conductivity of water compressed dynamically to pressures of 70–180 GPa (0.7–1.8 Mbar)The Journal of Chemical Physics, 2001
- Saturn Helium Abundance: A Reanalysis of Voyager MeasurementsIcarus, 2000
- Measurements of the Equation of State of Deuterium at the Fluid Insulator-Metal TransitionScience, 1998
- A Nongray Theory of Extrasolar Giant Planets and Brown DwarfsThe Astrophysical Journal, 1997
- Solar models with helium and heavy-element diffusionReviews of Modern Physics, 1995
- The helium abundance of Saturn from Voyager measurementsThe Astrophysical Journal, 1984
- The helium abundance of Jupiter from VoyagerJournal of Geophysical Research, 1981
- Phase separation of highly dissymmetric binary ionic mixturesPhysica A: Statistical Mechanics and its Applications, 1979