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X-ray emission from the Magellanic Clouds observed by Uhuru.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.
Document ID
19720028529
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/180842
Authors
Leong, C.
Kellogg, E.
Gursky, H.
Tananbaum, H.
Giacconi, R. (American Science and Engineering, Inc. Cambridge, Mass., United States)
Date Acquired
August 6, 2013
Publication Date
December 1, 1971
Publication Information
Publication: Astrophysical Journal
Volume: 170
Subject Category
Space Sciences
Accession Number
72A12195
Funding Number(s)
CONTRACT_GRANT: NAS5-11422
Distribution Limits
Public
Copyright
Other

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