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HEAO 1 high-energy X-ray observations of Centaurus X-3Pulsations of 4.8 sec were detected up to energies above 38 keV by the present High Energy X-ray and Low Energy Gamma-Ray HEAO 1 satellite experiment observations of Cen X-3, and an analysis of the X-ray spectrum as a function of pulse phase indicates that the spectrum hardens during an interval of about 1.2 sec which lags the pulse peak by about 0.6 sec. The results of correlated observations of pulse period and X-ray intensity include (1) the detection of a high intensity state during which the pulse period is on the average increasing, (2) the measurement of comparable high intensities during episodes of both period increase and decrease, (3) the detection of X-ray pulsations at a much reduced level during a period of low intensity, and (4) the detection of a transition between spin-down, and spin-up episodes that coincides with a rapid decrease in X-ray intensity.
Document ID
19830065778
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Howe, S. K.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Primini, F. A.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Bautz, M. W.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Lang, F. L.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Levine, A. M.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Lewin, W. H. G.
(MIT Cambridge, MA, United States)
Date Acquired
August 11, 2013
Publication Date
September 15, 1983
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 272
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
83A46996
Funding Number(s)
CONTRACT_GRANT: NAS8-27975
Distribution Limits
Public
Copyright
Other

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