Fig. 12 from The Spitzer Survey of the Small Magellanic Cloud: S3MC Imaging and Photometry in the Mid‐ and Far‐Infrared Wave Bands

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The Spitzer Survey of the Small Magellanic Cloud: S³MC Imaging and Photometry in the Mid‐ and Far‐Infrared Wave Bands

Authors: Alberto D. Bolatto, Joshua D. Simon, Snežana Stanimirović, Jacco Th. van Loon, Ronak Y. Shah, Kim Venn, Adam K. Leroy, Karin Sandstrom, James M. Jackson, Frank P. Israel, Aigen Li, Lister Staveley-Smith, Caroline Bot, Francois Boulanger, and Mónica Rubio

Bolatto et al. 2007 The Astrophysical Journal 655 212.

Provider: AAS Journals

Caption: Fig. 12.

Color‐color plots in the Spitzer and 2MASS wave bands. The color of the symbols is identical to that employed in Figs. 9 and 10. Panels (a), (b), and (c) show plots similar to those modeled by Whitney et al. (2003) for a variety of sources. The group 1 sources (green symbols) fall into the locii of Class 0 to Class II YSOs. Panel (d), a plot similar to Fig. 1 of Sloan et al. (2006), clearly shows the two sequences of silicate and carbon‐rich dusty evolved stars (red symbols).

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