7Li/6Li and 11B/10B variations in chondrules from the Semarkona unequilibrated chondrite
- 30 December 1998
- journal article
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 164 (3-4) , 577-589
- https://doi.org/10.1016/s0012-821x(98)00250-7
Abstract
No abstract availableKeywords
This publication has 34 references indexed in Scilit:
- Interstellar water in meteorites?Published by Elsevier ,2000
- Interstellar hydroxyl in meteoritic chondrules: implications for the origin of water in the inner solar systemGeochimica et Cosmochimica Acta, 1998
- Light Isotopes, Extinct Radioisotopes, and Gamma-Ray Lines from Low-Energy Cosmic-Ray InteractionsThe Astrophysical Journal, 1996
- Nucleosynthesis of 11B-rich boron in the pre-solar cloud recorded in meteoritic chondrulesNature, 1995
- Production and evolution of light elements in active star-forming regionsNature, 1995
- On the origin of the light elements ()Reviews of Modern Physics, 1994
- The isotopic composition of cosmic-ray B, C, N, and O - Evidence for an overabundance of O-18The Astrophysical Journal, 1992
- Petrology and mineralogy of Type II, FeO-rich chondrules in Semarkona (LL3.0): Origin by closed-system fractional crystallization, with evidence for supercoolingGeochimica et Cosmochimica Acta, 1990
- Deuterium/hydrogen ratios in unequilibrated ordinary chondritesNature, 1981
- Galactic Cosmic Ray Origin of Li, Be and B in StarsNature, 1970