Figure 9 from Discovery and Analysis of 21 μm Feature Sources in the Magellanic Clouds

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Discovery and Analysis of 21 μm Feature Sources in the Magellanic Clouds

Authors: Kevin Volk, Bruce J. Hrivnak, Mikako Matsuura, Jeronimo Bernard-Salas, Ryszard Szczerba, G. C. Sloan, Kathleen E. Kraemer, Jacco Th. van Loon, F. Kemper, Paul M. Woods, Albert A. Zijlstra, Raghvendra Sahai, Margaret Meixner, Karl D. Gordon, Robert A. Gruendl, Alexander G. G. M. Tielens, Remy Indebetouw, and Massimo Marengo

Volk et al. 2011 The Astrophysical Journal 735 127.

Provider: AAS Journals

Caption: Figure 9.

Continuum divided UIR profiles for the objects are shown normalized to a peak height of 1.0 for the 6.3 μm feature. The upper panel shows the short-wavelength region with the 6.3, 6.9, 7.7, and 8.6 μm features. The lower panel shows the 10–19 μm region, illustrating the wide range of relative strengths of the 11.2 μm feature compared to the normalized 6.3 μm features. Additional features are marked at 12.2, 13.2, and 15.8 μm.

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