1998ApJ...507L..63W

We analyzed the rapid aperiodic X-ray variability of the recently discovered millisecond X-ray pulsar SAX J1808.4-3658. The power density spectrum is dominated by a strong band-limited noise component, which follows a power law with index 1.0-1.3 at high frequencies with a break that varies between 0.25 and 1.6 Hz, below which the spectrum is relatively flat. Superimposed on this, a broad bump is present with a centroid frequency that varies well correlated with the break frequency between 2.4 and 12.0 Hz. These characteristics are very similar to what is commonly seen in other low-luminosity low-mass X-ray binaries. Between 100 and 400 Hz, a third broad noise component is present similar to that recently reported in the low-luminosity low-mass X-ray binary 4U 1728-34 (Ford & van der Klis). We find a similar high-frequency noise component also in other low-luminosity neutron star systems. We conclude that at any given epoch, the rapid aperiodic X-ray variability of the millisecond X-ray pulsar is indistinguishable from that of other low-luminosity neutron star systems. However, contrary to what has been found in those sources, the break frequency of the band-limited noise does not have a strict correlation with mass accretion rate. With decreasing mass accretion rate, the break frequency first decreased, then increased again. This previously unobserved behavior could be typical for the very low mass accretion rates we observe near the end of the outburst of SAX J1808.4-3658, or it could be related to its being a pulsar.