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Quasi-periodic oscillations in the Z source GX 5-1A detailed study has been conducted of the time variability in the Z source GX 5-1 using Ginga, which observed the source in the horizontal and normal branches (HB, NB). Intensity-dependent HF, quasi-periodic oscillations (QPO) were observed in the HB, in which the source flux varied by a factor of 1.9. The QPO frequency in this portion of the HB ranges from about 13 to 17 Hz; this is lower than previously observed in any Z source. The HF and LF QPO were simultaneously observed in the NB. The strength of both forms of QPO and the strength of the LF noise increase rapidly with increasing photon energy.
Document ID
19920060952
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lewin, Walter H. G.
(MIT Cambridge, MA, United States)
Lubin, Lori M.
(MIT, Cambridge, MA; Princeton University NJ, United States)
Tan, Jianmin
(MIT Cambridge, MA, United States)
Van Der Klis, Michiel
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Van Paradijs, Jan
(Amsterdam, University; Center for High Energy Astrophysics, Netherlands)
Penninx, Wim
(Amsterdam, University; Center for High Energy Astrophysics; Delft, Technical University, Netherlands)
Dotani, Tadayasu
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Mitsuda, Kazuhisa
(Institute of Space and Astronautical Science Sagamihara, Japan)
Date Acquired
August 15, 2013
Publication Date
June 15, 1992
Publication Information
Publication: Royal Astronomical Society, Monthly Notices
Volume: 256
Issue: 4 Ju
ISSN: 0035-8711
Subject Category
Astrophysics
Accession Number
92A43576
Funding Number(s)
CONTRACT_GRANT: NSG-7643
CONTRACT_GRANT: NAG8-571
CONTRACT_GRANT: NATO-RG-331/88
CONTRACT_GRANT: NAG8-674
Distribution Limits
Public
Copyright
Other

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