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As part of a continuing study of the effect of cluster environment on thestar formation properties of galaxies, we have undertaken an H-alpha objectiveprism survey of the nearby cluster, Abell 1060. We detect 33 galaxies inemission, 24 of which are cluster members. We present new radial velocitymeasurements and H-alpha+[NII] equivalent widths and fluxes for a number ofthese galaxies. We distinguish between galaxies with diffuse and compactemission, the latter having been associated in previous work with a disturbedmorphology of the galaxy and most likely resulting from tidally-induced starformation from galaxy-galaxy or cluster-galaxy interactions. The fraction ofcluster spirals in Abell 1060 detected with compact emission agrees with theexpected fraction for a cluster of its richness, as derived from results of aprevious survey of 8 clusters. Some of the detected cluster early-type spiralsexhibit anomalously high global H-alpha equivalent widths, as compared togalaxies of similar type in the field.Comment: 10 pages, Latex, 2 figures, needs l-aa macros. Accepted for  publication in Astronomy and Astrophysics Supplement Serie

Hα objective prism survey of Abell 1060