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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 2.

Examples of the methodology employed to identify spatially extended emission with respect to the MIRI PSF. On top are the spaxel-by-spaxel, continuum-subtracted, intensity-integrated maps of the mentioned lines, where the blue stars represent the centroids of the corresponding continuum. For GY92-21, two maps are shown, one before rescaling the emission and one after (see Section 3.1 for details). On the bottom are the encircled-flux curves as described in the main text, with the conclusion about the emission’s extent written in the top left.

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