Color Figures for

``The Pleiades Reflection Nebula: II. Simple Model Constraints on Dust Properties and Scattering Geometry''

Gibson, S. J., & Nordsieck, K. H. 2003, Ap.J., 589, 362


Figure 1. Interstellar reddening and molecular gas distributions across the cluster core.


Figure 2. Simple reflection nebula cartoon.


Figure 3. Scattering geometry illustration.


Figure 4. Maps of scattering angle in the cluster core for standard GCW grains and a Model A nebula (left) and UV-altered GCW grains in the same model (right).


Figure 5. Degrees of consistency between the scattering angles of different models at different wavelengths.


Figure 6. Dust properties vs. wavelength for different models.


Figure 7. Comparison with (a, g) values from the literature.


Figure 8. Schmidt scattering angles over a wider area.


Figure 9. Schmidt line-of-sight separations over the same area, derived for two different simplified geometric models.


Figure 10. Comparison of nebular intensities with multiple illuminator model.


Figure 11. Ratio of Schmidt / model with nebular gas H I 21cm contours overlaid.