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NEW ULTRAVIOLET EXTINCTION CURVES FOR INTERSTELLAR DUST IN M31

  • Authors: Geoffrey C. Clayton, Karl D. Gordon, Luciana C. Bianchi, Derck L. Massa, Edward L. Fitzpatrick, R. C. Bohlin, and Michael J. Wolff

2015 The Astrophysical Journal 815 14.

  • Provider: AAS Journals

Caption: Figure 3.

Extinction curves for the target sample using the best fits with atmosphere models. The extinction curves are J003944.71+402056.2 (upper left), J003958.22+402329.0 (upper right), J004034.61+404326.1 (lower left), and J004412.17+413324.2 (lower right). The black line is the extinction curve using STIS spectra, and the black squares are UBVRI. Shown for comparison are the SMC average extinction curve (blue), the LMC (30-Dor) average extinction curve (green), and the MW CCM R(V) = 3.1 (red). The best fit to the FM parameters, listed in Table 5, is represented by the red dashed line.

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