Figure 10 from The Spitzer Infrared Spectrograph Survey of T Tauri Stars in Taurus

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The Spitzer Infrared Spectrograph Survey of T Tauri Stars in Taurus

Authors: E. Furlan, K. L. Luhman, C. Espaillat, P. D'Alessio, L. Adame, P. Manoj, K. H. Kim, Dan M. Watson, W. J. Forrest, M. K. McClure, N. Calvet, B. A. Sargent, J. D. Green, and W. J. Fischer

Furlan et al. 2011 The Astrophysical Journal Supplement Series 195 3.

Provider: AAS Journals

Caption: Figure 10.

Equivalent width of the 10 μm silicate feature vs. the spectral type for the T Tauri stars in our sample. The "outliers" from Figure 8 (those objects that cannot be described by full accretion disks; see the text) are shown with star symbols. For each spectral type, a square is plotted at the median EW(10 μm) value. The dashed line represents a linear fit to the data shown.

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