Southwestern part of Bar as seen by the JWST’s MIRI instrument with north up and east left. Several images in different filters were combined to produce an RGB composite image: F1500W (green), F1130W (blue) and F770W (red) that traces respectively continuum emission from hot/warm dust and hydrocarbons (AIBs). The individual images used to make the RGB composite one are shown below. The size of the images is ~42″ × 42″ and it is centered on RA=05^h35^m20^s.33, DEC=-05°25′03.77″ very close the irradiated proto-planetary disk 203-504.