A dendritic solidification model to explain Ge-Ni variations in iron meteorite chemical groups
- 1 February 1982
- journal article
- Published by Elsevier in Geochimica et Cosmochimica Acta
- Vol. 46 (2), 259-268
- https://doi.org/10.1016/0016-7037(82)90253-8
Abstract
No abstract availableThis publication has 20 references indexed in Scilit:
- Experimental determination of ternary partition coefficients in Fe-Ni-X alloysMetallurgical Transactions A, 1981
- Chemical classification of iron meteorites—IX. A new group (IIF), revision of IAB and IIICD, and data on 57 additional ironsGeochimica et Cosmochimica Acta, 1980
- Cooling rates of seven hexahedritesGeochimica et Cosmochimica Acta, 1978
- Chemical fractionations in meteorites—VIII. Iron meteorites and the cosmochemical history of the metal phaseGeochimica et Cosmochimica Acta, 1977
- The chemical classification of iron meteorites. VI. A reinvestigation of irons with Ge concentration lower than 1 ppmIcarus, 1972
- The ternary phase diagram, Fe-Ni-PMetallurgical Transactions, 1970
- The iron meteorites, their thermal history and parent bodiesGeochimica et Cosmochimica Acta, 1967
- Origin, age, and composition of meteoritesSpace Science Reviews, 1964
- The distribution of gallium, germanium, cobalt, chromium, and copper in iron and stony-iron meteorites in relation to nickel content and structureGeochimica et Cosmochimica Acta, 1957
- The distribution of nickel, cobalt, gallium, palladium and gold in iron meteoritesGeochimica et Cosmochimica Acta, 1951