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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. 11.

5780 Å (top), 5797 Å (middle), and 6284 Å (bottom) DIBs vs. N(H I) (left) and E(BV) (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 0.9{\mbox{--}} 1.3﹩ vs. N(H I) and ~0.8–1.1 vs. E(BV); omitting "discrepant" sight lines].

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