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Interstellar Grains in Museums?

Published online by Cambridge University Press:  14 August 2015

A. G. W. Cameron
A. G. W. Cameron*
Affiliation:
Belfer Graduate School of Science, Yeshiva University, New York, N.Y., U.S.A.Goddard Institute for Space Studies, NASA, New York, N.Y., U.S.A.

Abstract

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It is argued that carbonaceous chondrites, particularly of type I, are probably collections of interstellar grains which have been mildly transformed through exposure to higher than normal temperatures, resulting in a loss of volatile materials.

Information

Type
Part X Miscellaneous
Information
Symposium - International Astronomical Union , Volume 52: Interstellar Dust and Related Topics , 1973, pp. 545 - 547
Copyright
Copyright © Reidel 1973 

References

Brecher, A.: 1972, ‘On the Primordial Condensation and Accretion Environment and the Remanent Magnetism of Meteorites’, in Proc. IAU Symposium on the Evolutionary and Physical Properties of Meteoroids , in press.CrossRefGoogle Scholar
Cameron, A. G. W.: 1973, Icarus 18, 407–450.CrossRefGoogle Scholar
Cameron, A. G. W. and Pine, M. R.: 1973, Icarus 18, 377–406.CrossRefGoogle Scholar
Huffman, D. R. and Stapp, J. L.: 1973, this volume, p. 297.CrossRefGoogle Scholar
Larson, R. B.: 1969, Monthly Notices Roy. Astron. Soc. 145, 271–295.CrossRefGoogle Scholar