Figure 6 from DirtyGrid I: 3D Dust Radiative Transfer Modeling of Spectral Energy Distributions of Dusty Stellar Populations

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DirtyGrid I: 3D Dust Radiative Transfer Modeling of Spectral Energy Distributions of Dusty Stellar Populations

Authors: Ka-Hei Law, Karl D. Gordon, and Karl A. Misselt

2018 The Astrophysical Journal Supplement Series 236 32.

Provider: AAS Journals

Caption: Figure 6.

Optical V band flux vs. optical depth for three stellar ages (1, 100, and 13,000 Myr) and three clumpy geometries (Shell, Dusty, and Cloudy). In general, band integrated fluxes vary smoothly with optical depth. The smoothness enables the use of interpolation to greatly reduce the number of optical depths needed.

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