Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

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 8.

Histogram of mass accretion rates for sources with extended H2 winds detected in S(1) (blue), S(5) (orange), and S(7) (red). Multiple-star systems are excluded, and so are several highly inclined disks (i > 80∘) lacking reliable accretion rate measurements (Table 1).

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse