NASA NTRS · 19720028529
X-ray emission from the Magellanic Clouds observed by Uhuru.
Abstract
Description of three sources in the Large Magellanic Cloud and one in the Small Cloud which have been discovered by Uhuru. These sources each emit about 10 to the 38th erg/sec in the 2- to 7-keV band, and they account for more than 90% of the total emission from the Clouds. The source in the Small Cloud shows time variability on time scales of hours.
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Leong, C., Kellogg, E., Gursky, H., Tananbaum, H., Giacconi, R.. 1971-12-01. X-ray emission from the Magellanic Clouds observed by Uhuru.. https://ntrs.nasa.gov/citations/19720028529
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