Evidence for Widespread 26 Al in the Solar Nebula and Constraints for Nebula Time Scales-Reference-Cited by-同舟云学术

Evidence for Widespread 26 Al in the Solar Nebula and Constraints for Nebula Time Scales

Published:1996-08-09 Issue:5276 Volume:273 Page:757-762
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Russell S. S.¹,Srinivasan G.²,Huss G. R.²,Wasserburg G. J.²,MacPherson G. J.¹

Affiliation:

1. S. S. Russell and G. J. MacPherson are in the Department of Mineral Sciences, MRC NHB-119, National Museum of Natural History, Smithsonian Institution, Washington, DC 20560, USA.

2. G. Srinivasan, G. R. Huss, and G. J. Wasserburg are in the Lunatic Asylum, Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference35 articles.

1. BERNIUS M.T., LUNAR PLANET SCI 22, 93 (1991).

2. AL-RICH OBJECTS IN ORDINARY CHONDRITES - RELATED ORIGIN OF CARBONACEOUS AND ORDINARY CHONDRITES AND THEIR CONSTITUENTS;BISCHOFF A;GEOCHIMICA ET COSMOCHIMICA ACTA,1984

3. BRIGHAM C.A., THESIS CALTECH (1990).

4. THE FIRST 10-MILLION YEARS IN THE SOLAR NEBULA;CAMERON AGW;METEORITICS,1995

5. ABSOLUTE ISOTOPIC ABUNDANCE RATIOS AND ATOMIC WEIGHT OF MAGNESIUM;CATANZARO E.J.;JOURNAL OF RESEARCH OF THE NATIONAL BUREAU OF STANDARDS SECTION A-PHYSICS AND CHEMISTRY,1966

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