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The field of the globular cluster NGC 6362 was monitored between 1995 and2009 in a search for variable stars. BV light curves were obtained for 69periodic variables including 34 known RR Lyr stars, 10 known objects of othertypes and 25 newly detected variables. Among the latter we identified 18proper-motion members of the cluster: seven detached eclipsing binaries (DEBs),six SX Phe stars, two W UMa binaries, two spotted red giants, and a veryinteresting eclipsing binary composed of two red giants - the first example ofsuch a system found in a globular cluster. Five of the DEBs are located at theturnoff region, and the remaining two are redward of the lower main sequence.Eighty-four objects from the central 9x9 arcmin^2 of the cluster were found inthe region of cluster blue stragglers. Of these 70 are proper motion (PM)members of NGC 6362 (including all SX Phe and two W UMa stars), and five arefield stars. The remaining nine objects lacking PM information are located atthe very core of the cluster, and as such they are likely genuine bluestragglers.

The Clusters AgeS Experiment (CASE). Variable stars in the field of the globular cluster NGC 6362