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   51129
   We propose the X-ray spectroscopy of three Wolf-Rayet (W-R) starburst
   galaxies in order to search for the hard X-ray emission from AGN and to
   investigate the properties of the hot plasma. Previous optical studies
   on the W-R galaxies indicate that the star formation in the starburst
   galaxies occurs instantaneously with duration time of less than 1e6
   years. Thus, by selecting the W-R galaxies, we can study the star-
   formation activity in its most early and intense phase. We search for
   the hard X-ray emission which, if present, would provide evidence for
   the Warmer (Terlevich and Mernick 1985). We also analyze the
   temperature and metallicity of the host plasma to study their
   evolutionary change within the starburst phase by comparing with other
   starburst galaxies.
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