Timing an Accreting Millisecond Pulsar: Measuring the Accretion Torque in IGR J00291+5934

Details Timing an Accreting Millisecond Pulsar: Measuring the Accretion Torque in IGR J00291+5934 Timing an Accreting Millisecond Pulsar: Measuring the Accretion Torque in IGR J00291+5934

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006chjas...6a.192b&link_type=abstract

Chinese Journal of Astronomy and Astrophysics, Supplement, Volume 6, Issue S1, pp. 192-196 (2006).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We present here a timing analysis of the fastest accreting millisecond pulsar IGR J00291+5934 using RXTE data taken during the outburst of December 2004. We corrected the arrival times of all the events for the orbital (Doppler) effects and performed a timing analysis of the resulting phase delays. In this way we find a clear parabolic trend of the pulse phase delays showing that the pulsar is spinning up as a consequence of accretion torques during the X-ray outburst. The accretion torque gives us for the first time an independent estimate of the mass accretion rate onto the neutron star, which can be compared with the observed X-ray luminosity. We also report a revised value of the spin period of the pulsar.

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