Spatial comparison between MUSE stellar continuum (colormap) and MUSE emission lines (contours) for proplyds 154–346, 167–325, 168–326, 170–249, 170–334, 170–337, 171–340, 173–236, 174–414, 177–341W, 203–504, and 244–440. The emission line and the size of each image are shown in the top left corner. The contours represent 50%, 70%, and 90% of the peak intensity of the MUSE emission lines, except for the [C I] line of 174–414 for which only 90% is shown. The direction of the UV source is shown with an arrow.