Fig. 7 from Magellanic Cloud–Type Interstellar Dust along Low‐Density Sight Lines in the Galaxy

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Magellanic Cloud–Type Interstellar Dust along Low‐Density Sight Lines in the Galaxy

Authors: Geoffrey C. Clayton, Karl D. Gordon, and Michael J. Wolff

Clayton, Gordon, & Wolff 2000 The Astrophysical Journal Supplement Series 129 147.

Provider: AAS Journals

Caption: Fig. 7.

Comparison of the average SD region and non–SD region curves, as described in Fig. 6, with curves for the average MW (﹩R_{V}=3.1﹩), LMC average, LMC 2 shell, SMC bar, and SMC AzV 456.

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