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During the UIT/Astro Spacelab missions, the Ultraviolet Imaging Telescopeobtained spatially resolved far-UV (lambda 1500 A) imagery of ~35 galaxiesexhibiting recent massive star formation. The sample includes disk systems,irregular, dwarf, and blue compact galaxies. The objects span an observed FUVluminosity range from -17 to -22 magnitudes. We estimate global star formationrates by comparing the observed FUV fluxes to the predictions of stellarpopulation models, and compare the FUV-derived astration rates to those derivedfrom H-alpha and far-IR photometry.Comment: 4 pages, LaTeX, 2 encapsulated Postscript figures, using AIP Press  aipproc style file. Paper to appear in "Star Formation Near and Far",  Proceedings of the 7th annual Astrophysics Conference in Marylan

Luminosities and star formation rates of galaxies observed with the ultraviolet imaging telescope: A comparison of far-UV, Hα, and far-IR diagnostics