Figure 3 from Radial Gradients in Dust-to-gas Ratio Lead to Preferred Region for Giant Planet Formation

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Radial Gradients in Dust-to-gas Ratio Lead to Preferred Region for Giant Planet Formation

Authors: Yayaati Chachan, Eve J. Lee, and Heather A. Knutson

2021 The Astrophysical Journal 919 63.

Provider: AAS Journals

Caption: Figure 3.

Rosseland mean opacity per gram of dust for a power-law grain size distribution with β = −3.5 and −2.5 and three different temperatures. The lowest value of a_max = 0. 25 μm on this plot is the commonly adopted value for the ISM size distribution.

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