M33 GALEX Images

 
NUV Fits Image, New WCS
FUV Fits Image, New WCS

The near-UV (top) and far-UV (bottom) GALEX images with improved WCS solution used in the paper analysis. The Fits files can be downloaded above as well! Note that only the hottest stars emit in the far-UV, and how boht UV images trace the spiral arms of the galaxy well. This is because the most massive stars (and hence also the youngest!) are preferentially born in the spiral arms, as this is where the newer star formation is concentrated.