Fig. 4 from Three‐dimensional Structure of the Milky Way Disk: The Distribution of Stars and Dust beyond 0.35 R⊙

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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. 4.

240 μm sky maps of the smoothed DIRBE data (top), the modeled emission (middle), and the relative difference between the modeled and observed emission (bottom). The top two maps are on a logarithmic scale, while the bottom map is on a linear scale.

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