Millihertz Oscillation Frequency Drift Predicts the Occurrence of Type I X-ray Bursts

Nov, 2007
5 pages
Published in:
  • Astrophys.J.Lett. 673 (2008) L35
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Abstract: (arXiv)
Millihertz quasi-periodic oscillations reported in three neutron-star low mass X-ray binaries have been suggested to be a mode of marginally stable nuclear burning on the neutron star surface. In this Letter, we show that close to the transition between the island and the banana state, 4U~1636--53 shows mHz QPOs whose frequency systematically decreases with time until the oscillations disappear and a Type I X-ray burst occurs. There is a strong correlation between the QPO frequency ν\nu and the occurrence of X-ray bursts: when ν9\nu\gtrsim9 mHz no bursts occur, while ν9\nu\lesssim9 mHz does allow the occurrence of bursts. The mHz QPO frequency constitutes the first identified observable that can be used to predict the occurrence of X-ray bursts. If a systematic frequency drift occurs, then a burst happens within a few kilo-seconds after ν\nu drops below 9 mHz. This observational result confirms that the mHz QPO phenomenon is intimately related with the processes that lead to a thermonuclear burst.