Generation of Type I X-ray Burst Oscillations by Unstable Surface Modes
arXiv:astro-ph/0702690 · doi:10.1086/519552
Abstract
The Rossi X-ray Timing Explorer has detected nearly coherent oscillations in the tails of type I X-ray bursts from 17 low-mass X-ray binaries. The oscillations are thought to be generated by brightness fluctuations associated with a surface mode on the rotating neutron star. The mechanism that drives the modes is, however, not understood, since the burning layer is stable to thermal perturbations. We show here via a linear perturbation analysis that, even under conditions when pure thermal perturbations are stable, nonradial surface modes may still be unstable by the epsilon mechanism. Specifically, we find that, if helium-burning reactions supply a reasonable fraction of the outgoing flux during burst decay, nonradial surface modes will grow in time. On the other hand, the same modes are likely to be stable in the presence of hydrogen burning via the rp-process. The results naturally explain why oscillations in the decay phase of type I X-ray bursts are detected only from short-duration bursts.
9 pages, accepted by ApJ
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- Multidimensional Modeling of Type I X-ray Bursts. I. Two-Dimensional Convection Prior to the Outburst of a Pure Helium Accretor
- NuSTAR observation of a Type I X-ray burst from GRS 1741.9-2853
- The accretion rate dependence of burst oscillation amplitude
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- Bursting behavior of the Galactic Center faint X-ray transient GRS 1741.9-2853
- NICER Observation of Unusual Burst Oscillations in 4U 1728-34
- Light curves from rapidly rotating neutron stars
- Damping of Type I X-ray Burst Oscillations by Convection