Fig. 13 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. 13.

Average SEDs of the different populations described in the main text. The SEDs were obtained as the median at each wavelength over the entire distribution of objects. The drop in the SED at 4.5 μm seen in carbon stars and RSG and OAGB stars is probably due to the CO fundamental band head at 4.7 μm seen in absorption.

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