Fig. 5 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. 5.

Left: Three‐color image of IRAS 04368+2557 using IRAC 3.6 μm (blue: 0–3 MJy sr⁻¹), IRAC 4.5 μm (green: 0–6 MJy sr⁻¹), and IRAC 7.8 μm (red: 0–12 MJy sr⁻¹). Right: Same image with the six photometry apertures overplotted (4^{﹩\arcsec﹩}, 8^{﹩\arcsec﹩}, 16^{﹩\arcsec﹩}, 32^{﹩\arcsec﹩}, 48^{﹩\arcsec﹩}, and 64^{﹩\arcsec﹩}).

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