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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. 6.

Extinction curves for the stars in the SD region (left) and in the rest of the sample (right) are plotted. Two sight lines, toward HD 151805 and 161653, in the SD region show normal CCM (﹩R_{V}=3.1﹩) extinction. The dust along those sight lines is not located in the same volume of space as the SD‐type dust, so they are plotted with the non–SD region sample.

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