Figure 12 from Discovery and Analysis of 21 μm Feature Sources in the Magellanic Clouds

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

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 12.

Percentage of the infrared emission in the 30 μm feature is plotted against the percentage of the infrared emission in the UIR features. Different sets of objects are plotted with different symbols: LMC objects (circles), SMC objects (squares), Galactic 21 μm objects re-fit the same way as the Magellanic Cloud objects (down triangles), and Galactic 21 μm objects with fits based on ISO spectra (from Hrivnak et al. 2000; up triangles). The dashed line shows the derived (weak) correlation function.

Other Images in This Article

Copyright and Terms & Conditions