Figure 4 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 4.

Relation between the crystalline-silicate indices, and the mass fractions of the corresponding crystalline minerals (upper) and amorphous large-grain material (lower), determined from the same spectra by fitting laboratory spectra (Sargent et al. 2006). The blue diamonds indicate the P ₁₀ index and orthoenstatite, and the magenta squares the O ₁₀ index and forsterite. The quality of linear fits to the data is indicated by the square of the linear correlation coefficient, r ² (see below, Equation 4).

Other Images in This Article

Copyright and Terms & Conditions