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DTSTART;TZID=Europe/Berlin:20180620T120000
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DTSTAMP:20260423T035042
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SUMMARY:ECAP Seminar: Frank Haberl
DESCRIPTION:The XMM-Newton surveys of the Magellanic Clouds\nUsing the XMM-Newton observatory\, we performed X-ray surveys of the Magellanic Clouds\, the two star-forming galaxies nearest to the Milky Way. The images obtained from the EPIC instruments provide a wealth of information about the X-ray source populations in the Small and Large Magellanic Cloud. Due to their proximity we can resolve the emission from supernova remnants\, and we have discovered many new X-ray binaries powered by accretion of matter. In particular the Small Magellanic Cloud is remarkable with respect to its large number of X-ray binaries with a high-mass donor star. These discrete sources are embedded in diffuse X-ray emission which originates in the hot phase of the interstellar medium of the clouds.
URL:https://ecap.nat.fau.de/index.php/event/ecap-seminar-frank-haberl/
LOCATION:ECAP\, room 307\, Erwin-Rommel-Str 1\, Erlangen\, 91058\, Germany
CATEGORIES:Seminar
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