Figure 9 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 9.

Histograms of the olivine indices, O ₁₀ (upper panel) and O ₃₃ (lower panel), for single stars and for multiple-star systems. Note the weak correlation of O ₁₀ with stellar multiplicity.

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