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Halfway to the Peak: Spatially Resolved Star Formation and Kinematics in a z = 0.54 Dusty Galaxy with JWST/MIRI

  • Authors: Jason Young, Alexandra Pope, Anna Sajina, Lin Yan, Thiago S Gonçalves, Miriam Eleazer, Stacey Alberts, Lee Armus, Matteo Bonato, Daniel A. Dale, Duncan Farrah, Carl Ferkinhoff, Christopher C. Hayward, Jed McKinney, Eric J. Murphy, Nicole Nesvadba, Patrick Ogle, Leonid Sajkov, Sylvain Veilleux

Jason Young et al 2023 The Astrophysical Journal Letters 958 .

  • Provider: AAS Journals

Caption: Figure 2.

Cutouts of the extracted spectrum around Brα (top) and [Ne II] (bottom), with best-fit Gaussian models. For [Ne II], red- and blueshifted components are shown, and one half of the peak-to-peak velocity differences are indicated. The tan curve at the bottom is the residual between the data and the continuum+Gaussian(s) model.

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