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JWST/MIRI Reveals the Evolution from Molecular to Atomic Disk Winds

  • Authors: Naman S. Bajaj, Ilaria Pascucci, Sylvie Cabrit, Suzan Edwards, Gabriele Cugno, Andrew D. Sellek, Joan R. Najita, Ke Zhang, Richard Alexander, Gregory J. Herczeg, Uma Gorti, Sophie C. Clark, Tracy L. Beck

Naman S. Bajaj et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 3.

This flowchart outlines our strategy to identify windlike H2 emission as described in Section 3.2. Only line maps that appear spatially resolved relative to the PSF in the flux curves (see Figure 2) are investigated for wind emission using this flowchart. Every line map shown in the flowchart is subtracted for continuum and integrated under a 1D Gaussian in every spaxel.

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