Journal Article

Type I X-ray bursts and burst oscillations in the accreting millisecond X-ray pulsar IGR J17511−3057

D. Altamirano, A. Watts, M. Linares, C. B. Markwardt, T. Strohmayer and A. Patruno

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 409, issue 3, pages 1136-1145
Published in print December 2010 | ISSN: 0035-8711
Published online December 2010 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2010.17369.x
Type I X-ray bursts and burst oscillations in the accreting millisecond X-ray pulsar IGR J17511−3057

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We report the discovery of burst oscillations at the spin frequency in ten thermonuclear bursts from the accreting millisecond X-ray pulsar (AMXP) IGR J17511−3057. The burst oscillation properties are, like those from the persistent AMXPs SAX J1808.4−3658 and XTE J1814−338, anomalous compared to burst oscillations from intermittent pulsars or non-pulsing low-mass X-ray binaries. Like SAX J1808.4−3658 they show frequency drifts in the rising phase rather than the tail. There is also evidence for harmonic content. Where IGR J17511−3057 is unusual compared to the other two persistent pulsars is that oscillations are not detected throughout all bursts. As accretion rate drops the bursts get brighter and their rise/decay time-scales become shorter, while the oscillation amplitude falls below the detection threshold: first in the burst peak and then also in the rise. None of the bursts from IGR J17511−3057 shows evidence for photospheric radius expansion (which might be expected to suppress oscillation amplitude) which allow us to set an upper limit to the distance of 6.9 kpc. We discuss the implications of our results for models of the burst oscillation mechanism.

Keywords: accretion, accretion discs; binaries: close; stars: individual: IGR J17511−3057; stars: neutron; pulsars: general; X-rays: stars

Journal Article.  6078 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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