REVISED ORBITAL PARAMETERS OF THE ACCRETING MILLISECOND PULSAR SAX J1808.4-3658

摘要

We present a temporal analysis of the three outbursts of the X-ray millisecond pulsar SAX J1808.4-3658 that occurred in 1998, 2000, and 2002. With a technique that uses the X~2 obtained with an epoch-folding search to discriminate between different possible orbital solutions, we find an unique solution valid over the whole 5 yr period for which high temporal resolution data are available. We revise the estimate of the orbital period, P_(orb) = 7249.1569(1) s, and reduce the corresponding error by 1 order of magnitude with respect to that previously reported. Moreover, we report the first constraint on the orbital period derivative, ― 6.6 x 10~(12) < P_(orb) < +0.8 x 10~(12) s s~(-1). These values allow us to produce, via a folding technique, pulse profiles at any given time. Analysis of these profiles shows that the pulse shape is clearly asymmetric in 2002, occasionally showing a secondary peak at about 145° from the main pulse, which is quite different from the almost sinusoidal shape reported at the beginning of the 1998 outburst.