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Spectroscopic observations of a massive star formation in the ultraviolet andtheir interpretation are reviewed. After a brief historical retrospective, twowell-studied resolved star clusters and the surrounding H II regions areintroduced: NGC 2070 in the Large Magellanic Cloud and NGC 604 in M33. Theseregions serve as a training set for studies of more distant clusters, which canno longer be resolved into individual stars. Observations of recently formedstar clusters and extended regions in star-forming galaxies in the nearbyuniverse beyond the Local Group are presented. Their interpretation relies onspectral synthesis models. The successes and failures of such models arediscussed, and future directions are highlighted. I present a case study of theextraordinary star cluster and giant H II region in the blue compact galaxy IIZw 40. The review concludes with a preview of two upcoming Hubble SpaceTelescope programs: ULLYSES, a survey of massive stars in nearby galaxies, andCLASSY, a study of massive star clusters in star-forming galaxies.

Massive Star Formation in the Ultraviolet Observed with the Hubble Space Telescope