Fig. 9 from VLT UVES Observations of Interstellar Molecules and Diffuse Bands in the Magellanic Clouds

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VLT UVES Observations of Interstellar Molecules and Diffuse Bands in the Magellanic Clouds

Authors: D. E. Welty, S. R. Federman, R. Gredel, J. A. Thorburn, and D. L. Lambert

Welty et al. 2006 The Astrophysical Journal Supplement Series 165 138.

Provider: AAS Journals

Caption: Fig. 9.

CH vs. K I (left) and CH vs. Na I (right). Circles denote LMC sight lines; triangles denote SMC sight lines; all other symbols are for Galactic sight lines (see Fig. 8). The solid lines show weighted and unweighted fits to the Galactic data (with ﹩\mathrm{slopes}\,\sim 1.0﹩; omitting "discrepant" sight lines).

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