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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 9.

Example DIRTY model output spectra showing the variations in each dimension of the parameter grid. In each plot, we vary one parameter and fix all the others. The fixed parameter values are 10 Myr old stellar age, 1010 solar masses, solar metallicity, instantaneous star formation, ﹩{\tau }_{V,\mathrm{ext}}=1﹩, Milky Way type dust, shell geometry, 10 kpc radius, and clumpy dust, except when shown in the legend of each plot.

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