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The Timing Evolution of 4U 1630-47 During its OutburstsWe report on the timing analysis of Rossi X-ray Timing Explorer (RXTE) observations of 4U 1630-47 made during its 1998 outburst. In addition we use two BeepoSAX observation on the late decline. 4U1630-47 showed seven distinct types of timing behaviour, most of which show differences with the canonical black hole spectral/timing states. In marked contrast to previous outbursts we find quasi periodic oscillation (QPO) signals during nearly all stages of the outburst. In addition to 2 to 13 Hz QPO slow 0.01Hz QPO are observed. These slow QPO can dominate the light curve as quasi-regular 5 sec, 9--16% deep dips. During these dips we track the behaviour of two QPO's; one remaining constant near 13.5 Hz and the other varying between 7 and 4 Hz. The evolution of the timing and the concurrent spectral changes are mapped using a combination harness-intensity and colour-colour diagrams.
Document ID
20040071160
Acquisition Source
Headquarters
Document Type
Other - Journal Issue
Authors
Dieters, S. W.
(Alabama Univ.)
Belloni, T.
(Institute of Astronomy Cambridge, United Kingdom)
Kuulkers, E.
(Space Research Organization Netherlands Utrecht, Netherlands)
Woods, P.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
vanParadijs, J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Cui, W.
(Utah Univ. Salt Lake City, UT, United States)
Swank, J. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Zhang, S.-N.
Date Acquired
August 21, 2013
Publication Date
November 1, 1999
Publication Information
Publication: Bulletin of the American Astronomical Society
Volume: 32
Subject Category
Astrophysics
Funding Number(s)
CONTRACT_GRANT: NAG5-7927
Distribution Limits
Public
Copyright
Other

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