期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 347, 期 4, 页码 L61-L65出版社
OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2004.07434.x
关键词
accretion, accretion discs; instabilities; galaxies : active; X-rays : binaries; X-rays : galaxies; X-rays : individual : SAX J18084-3658
The aperiodic X-ray variability in neutron star and black hole X-ray binaries (XRBs) and active galactic nuclei (AGN) shows a characteristic linear relationship between rms amplitude and flux, implying a multiplying together or 'coupling' of variability on different time-scales. Such a coupling may result from avalanches of flares, due to magnetic reconnection in an X-ray-emitting corona. Alternatively this coupling may arise directly from the coupling of perturbations in the accretion flow, which propagate to the inner emitting regions and so modulate the X-ray emission. Here, we demonstrate explicitly that the component of aperiodic variability that carries the rms-flux relation in the accreting millisecond pulsar SAX J1808.4-3658 is also coupled to the 401-Hz pulsation in this source. This result implies that the rms-flux relation in SAX J1808.4-3658 is produced in the accretion flow on to the magnetic caps of the neutron star, and not in a corona. By extension we infer that propagating perturbations in the accretion flow, and not coronal flares, are the source of the rms-flux relations and hence the aperiodic variability in other XRBs and AGN.
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