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Three‐dimensional Structure of the Milky Way Disk: The Distribution of Stars and Dust beyond 0.35 R

  • Authors: Ronald Drimmel and David N. Spergel

Drimmel & Spergel 2001 The Astrophysical Journal 556 181.

  • Provider: AAS Journals

Caption: Fig. 2.

Map of the ratio of the smoothed to unsmoothed data (top), and the estimated local error σ240 (bottom). The maps are Mollweide galactic projections for ﹩\vert b\vert < 30^{\circ }﹩, on logarithmic scales, indicated by the gray‐scale bars. Blanked pixels are regions excluded from the present analysis (see text). Positive Galactic longitudes are to the left of center.

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