Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-09-02
Astronomy and Astrophysics
Astrophysics
Proceedings of "Astrophysics with All-Sky X-Ray Observations", in press
Scientific paper
We review X-ray flux modulation from X-ray binaries on time scales corresponding to the orbital period and those at longer time scales (so called superorbital). Those modulations provide a powerful tool to constrain geometry of the accretion flow. The most common cause of the superorbital variability appears to be precession. We then discuss two specific examples of discoveries of a coupling between the two types of variability and their physical interpretation. One is Cyg X-1, a black-hole binary with a high-mass companion, in which case we find the presence of an accretion bulge formed by collision of the stellar wind with the outer edge of the precessing accretion disc. The other is 4U 1820-303, a neutron star accreting from a low-mass white dwarf, in which case we interpret the superorbital variability as accretion rate modulation induced by interactions in a triple stellar system. Then, the varying accretion rate leads to changes of the size of the accretion bulge in that system, obscuring the centrally-emitted X-rays.
Gierlinski Marek
Ibragimov A. A.
Poutanen Juri
Wen Linqing
Zdziarski Andrzej A.
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