Comparison of Galex images of NGC 40 with UVIT images. We note that the UVIT images provide better resolution and show structure in the nebula. The core of NGC 40 in F169M FUV Sapphire (top middle) is compared with N219M NUV B15 that shows mainly C II 2326 Å emission. C II image is very similar to low-excitation nebular line emissions seen in [S II] or [N II] (Meaburn et al. 1996) whereas F169M image shows several bright nebular condensations (also see Fig. 3). The axes are α and δ.