Figure 1 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 1.

Spitzer-IRS spectrum of IS Tau. At the top are also indicated the positions of the strongest mineral features expected in submicron dust grains, calculated from optical constants for α quartz (Wenrich & Christensen 1996), orthoenstatite (Jaeger et al. 1998), and forsterite (Fabian et al. 2001). At bottom, for comparison, is an ISO SWS spectrum of comet Hale-Bopp (Crovisier et al. 1997).

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