On the Submillimeter Opacity of Protoplanetary Disks

نویسنده

  • B. T. Draine
چکیده

Solid particles with the composition of interstellar dust and power-law size distribution dn/da ∝ a−p for a ≤ amax with amax & 3λ and 3 < p < 4 will have submm opacity spectral index β(λ) ≡ d lnκ/d ln ν ≈ (p−3)βism, where βism ≈ 1.7 is the opacity spectral index of interstellar dust material in the Rayleigh limit. For the power-law index p ≈ 3.5 that characterizes interstellar dust, and that appears likely for particles growing by agglomeration in protoplanetary disks, grain growth to sizes a & 3mm will result in β(1mm) . 1. Grain growth can naturally account for β ≈ 1 observed for protoplanetary disks, provided that amax & 3λ. Subject headings: planetary systems: protoplanetary disks dust, extinction, submillimeter

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تاریخ انتشار 2005