Figure 10 from Mapping the Interstellar Medium with Near-infrared Diffuse Interstellar Bands

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Mapping the Interstellar Medium with Near-infrared Diffuse Interstellar Bands

Authors: G. Zasowski, B. Ménard, D. Bizyaev, D. A. García-Hernández, A. E. García Pérez, M. R. Hayden, J. Holtzman, J. A. Johnson, K. Kinemuchi, S. R. Majewski, D. L. Nidever, M. Shetrone, and J. C. Wilson

Zasowski et al. 2015 The Astrophysical Journal 798 35.

Provider: AAS Journals

Caption: Figure 10.

Difference between the median observed W_DIB distribution in the Galactic disk and that predicted by the best-fitting smooth exponential disk model, as a function of projected midplane distance R_helio and vertical height above the plane Z of the stars. Each panel corresponds to the range of longitude indicated.

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