Hydrodynamic instability of the solar nebula in the presence of a planetary core
- 1 August 1974
- Vol. 22 (4) , 416-425
- https://doi.org/10.1016/0019-1035(74)90074-8
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- Models of the giant planetsIcarus, 1974
- Hydrogen Flash in StarsNature, 1973
- Accumulation processes in the primitive solar nebulaIcarus, 1973
- Numerical models of the primitive solar nebulaIcarus, 1973
- Chemical fractionations in meteorites—VI. Accretion temperatures of H-, LL- and E-chondrites, from abundance of volatile trace elementsGeochimica et Cosmochimica Acta, 1973
- Chemical fractionations in meteorites—V. Volatile and siderophile elements in achondrites and ocean ridge basaltsGeochimica et Cosmochimica Acta, 1972
- Chemical fractionations in meteorites—IV abundances of fourteen trace elements in L-chondrites; implications for cosmothermometryGeochimica et Cosmochimica Acta, 1971
- Structure of Jupiter: Chemical Composition, Contraction, and RotationThe Astrophysical Journal, 1970
- Primordial noble gases in separated meteoritic minerals—IGeochimica et Cosmochimica Acta, 1970
- On Spherically Symmetrical AccretionMonthly Notices of the Royal Astronomical Society, 1952