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An Updated Dust-to-Star Geometry: Dust Attenuation Does Not Depend on Inclination in 1.3 ≤z ≤2.6 Star-forming Galaxies from MOSDEF

  • Authors: Brian Lorenz, Mariska Kriek, Alice E. Shapley, Naveen A. Reddy, Ryan L. Sanders, Guillermo Barro, Alison L. Coil, Bahram Mobasher, Sedona H. Price, Jordan N. Runco, Irene Shivaei, Brian Siana, Daniel R. Weisz

Brian Lorenz et al 2023 The Astrophysical Journal 951 .

  • Provider: AAS Journals

Caption: Figure 6.

Attenuation in the V band vs. stellar mass (left) and UV slope (β) vs. stellar mass (right). Both A V and β are measured as the median of the fits to the SEDs of the individual galaxies in each group. A V and β appear to be similar for edge-on and face-on galaxies at fixed mass and SFR. We see a strong correlation in both A V and β with mass, but no residual trends with the axis ratio or SFR.

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