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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 10.

Gas-phase metallicity computed from O3N2 plotted against stellar mass for each of the eight groups. The points are colored by SFR. The measured metallicities show a clear mass–metallicity relation, as expected. At similar stellar mass, a higher SFR leads to a lower metallicity, also as expected.

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