088395

The Magellanic Clouds openParMCsclosePar harbour a large sample of Be-X-ray binaries openParBeXRBsclosePar at a moderate distance with low Galactic foreground absorption. In the course of the eROSITA all-sky surveys the MCs and the Magellanic Bridge openParMBclosePar are scanned frequently. This provides the unique opportunity to detect high-mass X-ray binary openParHMXBclosePar systems during outburst in the full Magellanic System openParMSclosePar comma as already demonstrated during the first survey openPareRASS1closePar. To continue our AO19 program openParwhich covers eRASS2 and eRASS3closePar comma we propose five 20 ks 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.