Figure 3 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 3.

Outline of the crystalline-silicate index extraction, using the spectrum of IS Tau as an example. In each frame is a calibrated spectrum, baseline fit, equivalent width per channel, and composite pristine spectrum, presented in the same manner as in Figure 2. The green bars are the bands within which the equivalent width per channel is summed for the indices centered at 9.2, 9.9, 11.1, 12.5, 21.7 and 33.6 μm, reading from left to right.

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