Fig. 7 from Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting Observed SEDs Using a Large Grid of Precomputed Models

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Interpreting Spectral Energy Distributions from Young Stellar Objects. II. Fitting Observed SEDs Using a Large Grid of Precomputed Models

Authors: Thomas P. Robitaille, Barbara A. Whitney, Remy Indebetouw, and Kenneth Wood

Robitaille et al. 2007 The Astrophysical Journal Supplement Series 169 328.

Provider: AAS Journals

Caption: Fig. 7.

Image of the best‐fit model to the IRAC data only for IRAS 04368+2557, shown in the same bands (IRAC 3.6, 4.5, and 7.8 μm) and with the same scaling as the image in Fig. 5.

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