Correlated X-ray spectral and fast-timing behaviour of 4U 1636-53

dc.creatorPrins, S.
dc.creatorvan der Klis, M.
dc.date1997-01-21
dc.date.accessioned2026-07-07T02:22:45Z
dc.date.available2026-07-07T02:22:45Z
dc.descriptionWe present a study of the persistent X-ray emission from the low-mass X-ray binary 4U 1636-53 based ont he entire archival EXOSAT ME data set. We per- formed a homogeneous analysis of all five EXOSAT observations in terms of the correlated rapid X-ray variability and X-ray spectral properties by means of power spectra, and colour-colour and hardness-intensity diagrams, respectively. Over the years we find similar patterns in the colour-colour and hardness-intensity diagrams, but small shifts in their postions occur. We find one case of an island-banana transition. On all but one occasion the differences in colour are smaller than 5%. Between the two 'island state' data sets, we find a shift of 8 % in the soft colour, which must be at least partly intrinsic. Clear correlations are present between the X-ray colours (which are governed by the mass accretion rate) and the power spectrum. With increasing mass accretion rate the fractional rms amplitude of the power-law shaped power spectral component that dominates the power spectra below ~1 Hz rises, while the band-limited noise component at higher frequencies drops. The cut-off frequency of the band-limited component increases whn its amplitude decreases. This is reminiscent of the behaviour of black hole candidates in the low state.
dc.descriptionAccepted by Astronomy and Astrophysics, 10 pages, Latex, uses l-aa, full version (including 8 figures) available at http://www.astro.uva.nl/preprints/preprints.html, AIAP preprint nr 60
dc.identifierhttps://arxiv.org/abs/astro-ph/9701149
dc.identifierhttp://arxiv.org/abs/astro-ph/9701149
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10991
dc.subjectAstrophysics
dc.titleCorrelated X-ray spectral and fast-timing behaviour of 4U 1636-53
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