Figure 10 from POWDERDAY: Dust Radiative Transfer for Galaxy Simulations

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POWDERDAY: Dust Radiative Transfer for Galaxy Simulations

Authors: Desika Narayanan, Matthew J. Turk, Thomas Robitaille, Ashley J. Kelly, B. Connor McClellan, Ray S Sharma, Prerak Garg, Matthew Abruzzo, Ena Choi, Charlie Conroy, Benjamin D. Johnson, Benjamin Kimock, Qi Li, Christopher C. Lovell, Sidney Lower, George C. Privon, Jonathan Roberts, Snigdaa Sethuram, Gregory F. Snyder, Robert Thompson, and John H. Wise

2021 The Astrophysical Journal Supplement Series 252 12.

Provider: AAS Journals

Caption: Figure 10.

RGB images corresponding to ﹩0.3,0.5﹩, and 1 μm colors from model LATTE for three different viewing angles. Dust lanes in the galaxy (here, the dust mass is tied to the metal mass as a model assumption) are visible. As in Figure 8, the model galaxy is set at 30 Mpc. Images generated following the Lupton et al. (2004) scalings.

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