Figure 23 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 23.

Comparison of the 6–13 μm and 13–31 μm spectral indices for models with stellar masses of 0.2 and 0.5 M _☉. For each model pair, the mass accretion rate, settling parameter epsilon , and inclination angle are the same. The dotted line represents a line with slope 1 and no offset, while the dashed line is a linear fit to the data.

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