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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 5.

Histograms of the crystalline indices P 10, O 10, and S 10, and of the equivalent widths of the 10 and 20 μm silicate complexes and the 33 μm olivine feature, W 10, W 20, and W 33.

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