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CECILIA: Direct O, N, S, and Ar Abundances in Q2343-D40, a Galaxy at z ∼ 3

  • Authors: Noah S. J. Rogers, Allison L. Strom, Gwen C. Rudie, Ryan F. Trainor, Menelaos Raptis, Caroline von Raesfeld

Noah S. J. Rogers et al 2024 The Astrophysical Journal Letters 964 .

  • Provider: AAS Journals

Caption: Figure 2.

T e [S III]–T e [O III] trends measured in z ∼ 0 extragalactic H II regions (gray diamonds; see Section 3) and dwarf galaxies (blue squares; see Section 3) and in D40 (green circle) at z ∼ 3. The Garnett (1992) photoionization model T e [S III]–T e [O III] relation is shown as the solid red line; the empirical scaling relation of Rogers et al. (2021) is provided as the solid blue line. The dotted line represents equal T e [S III] and T e [O III]. The T e measured in D40 agree with the T e trends of local ionized regions and the empirical T e T e scaling relation.

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