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 with low Galactic foreground absorption. However, thetransient nature of Be/Xray binaries complicates observations in Xrays.Serendipitous detections of bright outbursts provide rare chances for furtherinvestigation. We propose three triggered XMMNewton observations of new orunexplored systems to continue the buildup of a large statistical sample ofthese sources.
