Fig. 17 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. 17.

Predicted J‐band GP emission profiles at ﹩\vert l\vert < 90^{\circ }﹩ for an axisymmetric model and three spiral models, ﹩m=2﹩ and ﹩m=4﹩ logarithmic spiral models, and a sheared H II spiral model, plotted against the data (crosses).

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