Figure 10 from Crystalline Silicates and Dust Processing in the Protoplanetary Disks of the Taurus Young Cluster

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Crystalline Silicates and Dust Processing in the Protoplanetary Disks of the Taurus Young Cluster

Authors: Dan M. Watson, Jarron M. Leisenring, Elise Furlan, C. J. Bohac, B. Sargent, W. J. Forrest, Nuria Calvet, Lee Hartmann, Jason T Nordhaus, Joel D. Green, K. H. Kim, G. C. Sloan, C. H. Chen, L. D. Keller, Paola d'Alessio, J. Najita, Keven I. Uchida, and J. R. Houck

WATSON et al. 2009 The Astrophysical Journal Supplement Series 180 84.

Provider: AAS Journals

Caption: Figure 10.

Search for trends between the crystalline indices and the global properties of the systems. Plotted are the crystalline indices for pyroxene ( P ₁₀), olivine ( O ₁₀, O ₃₃) and silica ( S ₁₀), and the equivalent widths of the 10 and 20 μm silicate complexes ( W ₁₀ and W ₂₀), from Table 1, against the stellar luminosity, stellar mass, disk/star mass ratio, and accretion rate from Table 3.

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