Fig. 13.
Download original image
Left: Composite image based on three JWST/NIRCam blue filters (F090W, F115W, F150W) that show the stellar light from multiple young stellar clumps in CRISTAL-13, a main-sequence star-forming galaxy at z = 4.58. Overlaid are the integrated [C II] line emission (white contours; ) and the dust continuum (orange; ). The ALMA beam is shown in the lower right corner. Right: Cartoon representation of the distribution of the stellar clumps traced by JWST (blue and green), the cold gas traced by the [C II] line (red), and the dust continuum (orange). The properties of the stellar clumps are based on the SED modeling presented in Lines et al. (2025).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.