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Magnetorotational Instability in Protoplanetary Disks. II. Ionization State and Unstable Regions

  • Authors: Takayoshi Sano, Shoken M. Miyama, Toyoharu Umebayashi, and Takenori Nakano

Sano et al. 2000 The Astrophysical Journal 543 486.

  • Provider: AAS Journals

Caption: Fig. 10.

Relative abundances ﹩n( X) / n_{\mathrm{H}\,}﹩ of some representative particles for the case of ﹩f_{g}=10^{-4}﹩ as functions of the height ﹩\vert z\vert ﹩ from the midplane at ﹩r=1﹩ AU. The other parameters are the same as those of the fiducial model. The top panel shows the ionization rate ζ.

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