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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 4.

H2 S(3) line-intensity and continuum maps for FT Tau (incl. = 40﹩\mathop{.}\limits^{{\unicode{x000b0}}}﹩5) and SY Cha (incl. = 51﹩\mathop{.}\limits^{{\unicode{x000b0}}}﹩1). The blue stars show the continuum centroids, and the red dashed lines show the known disk PAs from literature ALMA results (Table 1).

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