The condensation with partial isolation (CWPI) model of condensation in the solar nebula
- 1 September 1998
- journal article
- Published by Wiley in Meteoritics & Planetary Science
- Vol. 33 (5) , 1123-1137
- https://doi.org/10.1111/j.1945-5100.1998.tb01717.x
Abstract
No abstract availableKeywords
This publication has 20 references indexed in Scilit:
- Condensation in the primitive solar nebulaPublished by Elsevier ,2003
- Models for the fractionation of moderately volatile elements in the solar nebulaMeteoritics & Planetary Science, 1996
- The Kaidun meteorite: Composition and origin of inclusions in the metal of an enstatite chondrite clastMeteoritics & Planetary Science, 1996
- Silica‐merrihueite/roedderite‐bearing chondrules and clasts in ordinary chondrites: New occurrences and possible originMeteoritics, 1994
- A unique, (almost) unaltered spinel-rich fine-grained inclusion in KainsazMeteoritics, 1992
- Abundances of the elements: Meteoritic and solarGeochimica et Cosmochimica Acta, 1989
- Chapter 25. Formation of Liquid and Condensation of Gas in the Primitive Solar NebulaProgress of Theoretical Physics Supplement, 1988
- Silica-bearing chondrules and clasts in ordinary chondritesGeochimica et Cosmochimica Acta, 1986
- Volatile element chemistry in the solar nebula: Na, K, F, Cl, Br, and PIcarus, 1980
- Formation of the solar nebulaIcarus, 1962