An Unusual Precursor Burst with Oscillations from Sax 51808.4-3658 Sudip

We report the finding of an unusual, weak precursor to a thermonuclear X-ray burst from the accreting millisecond pulsar SAX 51808.4-3658. The burst in question was observed on Oct. 19, 2002 with the Rossi X-Ray Timing Explorer (RXTE) proportional counter array (PCA). The precursor began M 1 s prior to the onset. of a strong radius expansion burst, lasted for about 0.4 s, and exhibited strong oscillations at the 401 Hz spin frequency. Oscillations are not detected in the M 0.5 s interval between the precursor and the main burst. The estimated peak photon flux and energy fluence of the precursor are about 1/25, and 1/500 that of the main burst, respectively. From joint spectral and temporal modeling, we find that an expanding burning region with a relatively low temperature on the spinning neutron star surface can explain the oscillations, as well as the faintness of the precursor with respect to the main part of the burst. We dicuss some of the implications of our findings for the ignition and spreading of thermonuclear flames on neutron stars. Subject headings: methods: data analysis stars: neutron techniques: miscellaneous X-rays: binaries X-rays: bursts X-rays: individual (SAX31808.4-3658)