Astrophysical Interesting Compound Grains Produced by a Gas Evaporation Method

Kaito, C.; Saito, Y.

doi:10.1007/978-94-011-3640-2_25

C. Kaito³ &
Y. Saito³

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 173))

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Abstract

Production methods of Fe₃0₄ grain and MgS grain have been introduced. Fe₃O₄ grain was produced in an Ar gas pressure range of 25 to 100 Torr by evaporating FeO powder. The growth of Fe₃0₄ have been discussed as the result of oxidation of Fe grains. MgS grain produced by the reaction of Mg and S vapors grew in the coagulation of tiny cubic sulfide.

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References

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Authors and Affiliations

Department of Electronics and Information Science, Kyoto Institute of Technology, Matsugasaki Sakyo-ku Kyoto 606, Japan
C. Kaito & Y. Saito

Authors

C. Kaito
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Y. Saito
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Editors and Affiliations

Aeronomie CNRS, Université Paris VI, Verrières-le-Buisson, France
A. C. Levasseur-Regourd
Osaka Sangyo University, Osaka, Japan
H. Hasegawa

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Kaito, C., Saito, Y. (1991). Astrophysical Interesting Compound Grains Produced by a Gas Evaporation Method. In: Levasseur-Regourd, A.C., Hasegawa, H. (eds) Origin and Evolution of Interplanetary Dust. Astrophysics and Space Science Library, vol 173. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3640-2_25

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DOI: https://doi.org/10.1007/978-94-011-3640-2_25
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-5616-8
Online ISBN: 978-94-011-3640-2
eBook Packages: Springer Book Archive

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