UNCOVER: The rest ultraviolet to near infrared multiwavelength structures and dust distributions of sub-millimeter-detected galaxies in Abell 2744

With the wavelength coverage, sensitivity, and high spatial resolution of JWST, it is now possible to peer through the dust attenuation to probe the rest-frame near infrared (NIR) and stellar structures of extremely dusty galaxies at cosmic noon (z~1-3). In this paper we leverage the combined ALMA and JWST/HST coverage in Abell 2744 to study the multiwavelength (0.5-4.4${\mu}$m) structures of 11 sub-millimeter (sub-mm) detected galaxies at z~0.9-3.5 that are fainter than bright "classical" sub-mm galaxies (SMGs); 7 of which are detected in deep X-ray data. While these objects reveal a diversity of structures and sizes, all are smaller and more concentrated towards longer wavelengths. Of the X-ray-detected objects, only two show evidence for appreciable AGN flux contributions (at ${\gtrsim}$2${\mu}$m). Excluding the two AGN-dominated objects, the smaller long wavelength sizes indicate that their rest-frame NIR light profiles, inferred to trace their stellar mass profiles, are more compact than their optical profiles. The sub-mm detections and visible dust lanes suggest centrally-concentrated dust is a key driver of the observed color gradients. Further, we find that more concentrated galaxies tend to have lower size ratios (rest-frame NIR to optical); this suggests that the galaxies with the most compact light distributions also have the most concentrated dust. The 1.2mm flux densities and size ratios of these 9 objects suggest that both total dust quantity and geometry impact these galaxies' multiwavelength structures. Upcoming higher resolution 1.2mm ALMA imaging will facilitate joint spatially-resolved analysis and will directly test the dust distributions within this representative sub-mm population.