Chapter 9 Condensation of Dust Particles : Part IV Physical Processes in the Solar Nebula : Origin of the Solar System
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概要
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The process of nucleation and grain growth is formulated on the basis of a theory of homogeneous nucleation. This formulation is applied to the grain formation in a cooling gas with the cosmic abundances. From the viewpoint that the raw materials of the bodies in the solar system are grains formed in various sites in space, including the primordial solar nebula, the nature of grains formed in the sites of astrophysical interest is discussed in connection with the physical conditions.
- 理論物理学刊行会の論文
- 1989-03-10
著者
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Kozasa T
Department On Physics Kyoto University
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Kozasa Takashi
Department Of Physics Faculty Of Science Kyoto University
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HASEGAWA Hiroichi
Department of Physics, Kyoto University
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Hasegawa Hiroichi
Department Of Physics And Chemistry Gakushuin University
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Hasegawa Hiroichi
Department On Physics Kyoto University
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HASEGAWA Hiroichi
Department on Physics, Kyoto University
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