Figure 7 from Crystalline Silicates and Dust Processing in the Protoplanetary Disks of the Taurus Young Cluster

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 7.

Trends among the emission features and their crystalline indices. Plotted are indices derived from features of pyroxene, olivine and silica ( P ₁₀, O ₃₃, and S ₁₀, respectively), the full width at half-maximum of the 10 μm silicate complex (Δλ ₁₀), the equivalent widths of the 10 and 20 μm silicate complexes ( W ₁₀ and W ₂₀), and two of the continuum spectral indices ( n _{6 − 13} and n _{13 − 31}),all plotted as functions of the olivine index O ₁₀. Upper limits are indicated by open symbols.

Other Images in This Article

Copyright and Terms & Conditions