Image Details
Caption: Figure 7.
Comparison of the surface brightness profiles and model fits for NGVS ﹩{g}^{{\prime} }﹩-band and HST/ACS F475W images of NGVS-UCD548. This object is embedded in nearby bright galaxy light, as shown in NGVS imaging, which makes it difficult to detect the outer envelope. But HST imaging reveals a two-component structure of NGVS-UCD548.
© 2026. The Author(s). Published by the American Astronomical Society.