  The bright Magellanic irregular galaxy NGC 4449 was observed by the
Ultraviolet Imaging Telescope (UIT) during the Astro-2 Spacelab mission in
March, 1995. Far ultraviolet (FUV) images at a spatial resolution of ~3 arcsec
show bright star-forming knots that are consistent with the general optical
morphology of the galaxy and are often coincident with bright H II regions.
Comparison of FUV with H-alpha shows that in a few regions, sequential star
formation may have occurred over the last few Myr. The bright star forming
complexes in NGC 4449 are superposed on a smooth, diffuse FUV background that
may be associated with the H-alpha "froth."
