Inverstigating hard X-ray transients in the Magellanic Clouds
收藏ESA Earth Online2026-06-22 收录
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The Magellanic Clouds harbour a large sample of Be/Xray binaries at a moderateand well known distance. The Galactic foreground absorption in this direction islow. The transient nature of Be/Xray binaries complicates the observing inXrays. Serendipitous detections of Be/Xray binaries in outburst provide rarechances for further investigation. We propose three triggered XMMNewtonobservations of new or unexplored systems to continue the build up of a largestatistical sample of these sources.
