Figure 13 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 13.

Impact of galaxy inclination angle on attenuation laws. Curves represent UV-NIR attenuation curves for model galaxy LATTE for nine viewing angles, with three particular angles highlighted in color that correspond to the images on the right (face on, edge on, and intermediary). Edge-on inclination angles display steeper normalized curves, while face-on views result in grayer (flatter) attenuation curves.

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