Timing the accretion flow around accreting millisecond pulsars

Details Timing the accretion flow around accreting millisecond pulsars Timing the accretion flow around accreting millisecond pulsars

2008-09-19

arxiv.org/abs/0809.3368v1

Astronomy and Astrophysics

Astrophysics

To be published in the proceedings of the workshop 'A Decade of Accreting Millisecond X-ray pulsars' (Amsterdam 14-18 April 20

Scientific paper

10.1063/1.3031189

At present, ten years after they were first discovered, ten accreting millisecond pulsars are known. I present a study of the aperiodic X-ray variability in three of these systems, which led to the discovery of simultaneous kHz quasi periodic oscillations in XTE J1807-294 and extremely strong broadband noise at unusually low variability frequencies in IGR J00291+5934. Furthermore, we classified SWIFT J1756.9-2508 as an atoll source and measured in its 2007 outburst spectral and variability properties typical of the extreme island state. I also give detailed estimates of the total fluence during the studied outbursts.

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