Image Details

Choose export citation format:

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 7.

ALMA and JWST cutout images for the ALMA PPOs that have a JWST counterpart in Figure 6. The color stretch of each cutout image is adjusted to visually represent the source clearly. The synthesized beam size (0﹩\mathop{.}\limits^{^{\prime\prime} }﹩027 at 1.3 mm; 0﹩\mathop{.}\limits^{^{\prime\prime} }﹩066 at 3 mm) of the ALMA images is added to estimate the size of the cutout image. Some JWST PSFs have empty pixels at the center due to saturation. Note that the systematic offset ﹩\sim 0\mathop{.}\limits^{^{\prime\prime} }04﹩ between the JWST and ALMA image is uncorrected here. The W51-IRS2 PPO #90 and #91 are excluded in this figure as they will be covered in Figure 9.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse