Fig. A.1.
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Multiwavelength view of NGC 2090. Top: FUV, Hα, optical g-band, and NIR 2MASS K-band images, tracing young massive stars and the underlying older stellar population. The red rectangle shows the JWST field of view. Bottom: JWST images in the F335M, F770W, and F2100W bands and CO map, highlighting PAH emission, warm dust continuum, and molecular gas, respectively.
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