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Effects of Radionuclides on the Ionization State of Protoplanetary Disks and Dense Cloud Cores

  • Authors: Toyoharu Umebayashi and Takenori Nakano

UMEBAYASHI & NAKANO 2009 The Astrophysical Journal 690 69.

  • Provider: AAS Journals

Caption: Figure 4.

Ionization rate ζ CR by cosmic rays coming from one side of the disk as a function of the depth χ from the disk surface. The abscissa is normalized by the attenuation length of cosmic rays λ CR ≈ 96 g cm −2, and the ordinate is normalized by the ionization rate at the disk surface ζ (0) CR/2 and the exponential attenuation factor exp(−χ/λ CR). The solid line shows the ionization rate obtained by numerical integration of Equation (A6). The ionization rates given by the empirical formula (A9) with γ = 1, 3/4, and 2/3 are also shown for some values of χ/λ CR by different marks.

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