Fig. 5 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. 5.

240 μm emission profile for the data (crosses) and model (diamonds) within 0﹩\fdg﹩17 of the GP (﹩b=0﹩), on a logarithmic scale (﹩\mathrm{log}\,D﹩).

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