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High-resolution X-ray observations of the Orion NebulaObservations of the Trapezium region in the Orion Nebula have been obtained with the high-resolution X-ray imaging instrument on the Einstein Observatory. At least 58 sources of the X-ray emission have been revealed, and all but two can be identified with visible stars. The strongest source is the star theta(1)C, which excites the emission nebula, and has an X-ray luminosity of 6 x 10 to the 32nd ergs/s. No strong X-ray emission has been observed from members of the infrared cluster embedded within the Orion molecular cloud.
Document ID
19820034163
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ku, W. H.-M.
(Columbia University New York, NY, United States)
Righini-Cohen, G.
(Columbia Univ. New York, NY, United States)
Simon, M.
(New York, State University Stony Brook, NY, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: Science
Volume: 215
Subject Category
Astrophysics
Accession Number
82A17698
Funding Number(s)
CONTRACT_GRANT: NAS8-30753
Distribution Limits
Public
Copyright
Other

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