Host phases and origin of noble gases in meteorites
- 1 July 1981
- journal article
- research article
- Published by Springer Nature in The Science of Nature
- Vol. 68 (7) , 341-353
- https://doi.org/10.1007/bf01058023
Abstract
No abstract availableKeywords
This publication has 54 references indexed in Scilit:
- Carbyne as a possible constituent of the interstellar dustMonthly Notices of the Royal Astronomical Society, 1980
- XENON, OSMIUM, AND LEAD FORMED IN O-SHELLS AND C-SHELLS OF MASSIVE STARSMeteoritics, 1980
- Aluminum-26 in the early solar system - Fossil or fuelThe Astrophysical Journal, 1977
- Correction [to “Demonstration of 26Mg excess in Allende and evidence for 26Al”]Geophysical Research Letters, 1976
- Extinct Superheavy Element in the Allende MeteoriteScience, 1975
- A Component of Primitive Nuclear Composition in Carbonaceous MeteoritesScience, 1973
- On the origins of trapped helium, neon and argon isotopic variations in meteorites—II. Carbonaceous meteoritesGeochimica et Cosmochimica Acta, 1972
- Neon and Xenon in Carbonaceous ChondritesPublished by Elsevier ,1968
- Isotopic Abundance Anomalies in the Solar SystemAnnual Review of Nuclear Science, 1967
- Origin, age, and composition of meteoritesSpace Science Reviews, 1964