086080

The Magellanic Clouds openParMCsclosePar harbour a large sample of Be-X-ray binaries at a moderate and well known distance with low Galactic foreground absorption. However comma their transient nature complicates observations in X-rays. During the eROSITA all-sky survey the MCs and the Magellanic Bridge openParMBclosePar between them will be scanned frequently. This provides the unique opportunity to detect high-mass X-ray binaries openParHMXBsclosePar during outburst in the full Magellanic System openParMSclosePar. We propose five triggered XMM-Newton observations of new or unexplored HMXBs in the MS. Our goal is to study their spectral and temporal properties comma to continue the build-up of large statistical samples of these sources in both clouds and in particular in the MB comma where Be-X-ray binaries have already been found.