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We present preliminary results from a study of the compact star clusterpopulations in three local luminous blue compact galaxies: ESO 185-IG 013, ESO350-IG 038 (a.k.a. Haro 11), and MRK 930. These systems show peculiarmorphologies and the presence of hundreds of SCs that have been produced by thepast, recent, and/or current starburst phases. We use a complete set of HSTimages ranging from the UV to IR for each galaxy. Deep images in V(WFPC2/f606w) and I (WFPC2/f814w) are used to capture most of the star clustercandidates up to the old ones (fainter) which have had, in the past, lesspossibility to be detected. The other bands are used in the SED fittingtechnique for constraining ages and masses. Our goals are to investigate theevolution of these three blue compact galaxies and the star cluster formationimpact on their star formation history.

Tracing the star formation history of three Blue Compact galaxies through the analysis of their star clusters