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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 7.

The difference in attenuation between the Balmer lines and stellar continuum, measured in the V band, plotted against stellar mass. Again, we see no effects with inclination. We also observe that galaxies with higher mass and SFR tend to have higher excess nebular attenuation than galaxies at lower masses.

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