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We present BV CCD-data for 11 intermediate-age LMC clusters; the mainconclusions are: 1. in the (V_to, V_cl,m) and (V-to, (V_to-V_cl,m)) planes themodels yield a good overall description of the data; 2. with the currentsample, it is impossible to firmly choose between "classical" and"overshooting" models; 3. the separation in colour between the MS band and theRed He-burning Clump is smaller than predicted by theoretical tracks; 4. theexistence of the so-called "RGB phase-transition (Renzini and Buzzoni 1986)seems to be confirmed.Comment: 62 pages, 37 figures and tables 6 to 16 available on request,  uuencoded compressed postscript file with tables 1-5 and 17-18 included, BAP  08-1994-020-OA

Globular clusters in the Magellanic Clouds. I. BV CCD photometry for 11 clusters