  Wolf-Rayet (WR) stars in the Magellanic Clouds (MCs) are ideal for studying
the production of X-ray emission by their strong fast stellar winds. We have
started a systematic survey for X-ray emission from WR stars in the MCs using
archival Chandra, ROSAT, and XMM-Newton observations. In Paper I, we reported
the detection of X-ray emission from 29 WR stars using Chandra ACIS
observations of 70 WR stars in the MCs. In this paper, we report the search and
analysis of archival ROSAT PSPC and HRI observations of WR stars. While useful
ROSAT observations are available for 117 WR stars in the MCs, X-ray emission is
detected from only 7 of them. The detection rate of X-ray emission from MCs WR
stars in the ROSAT survey is much smaller than in the Chandra ACIS survey,
illustrating the necessity of high angular resolution and sensitivity. LMC-WR
101-102 and 116 were detected by both ROSAT and Chandra, but no large long-term
variations are evident.
