Figure 4 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 4.

DIRTYGrid extinction curves for the MW, LMC 2, and SMC Bar dust models are shown. The primary differences between these curves are the strength of the 2175 Å bump and the far-UV rise. Our choice of dust types is intended to cover the range of dust properties observed in galaxies.

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