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A JWST NIRCam/MIRI View of the W51A High-mass Star-forming Region

  • Authors: Taehwa Yoo, Adam Ginsburg, Nazar Budaiev, Roberto Galván-Madrid, Aden Dawson, Savannah Gramze, Jesús Hernández, Alexandre Roman-Lopes, Carlos G. Román-Zúñiga, Joel Sanchez-Bermudez, Miriam G. Santa-Maria, Aida Wofford, Jason E. Ybarra

Taehwa Yoo et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 4.

Multiple color images of W51A region in a large-scale view. The images of F405N − F410M (top), F480M − F360M (middle), and F335M/F480M (bottom) are displayed to represent ionized gas, warm dust, and PAH abundance, respectively. The cyan contour marks the flux density of F405N − F410M image at 250 MJy sr−1.

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