Multiple X-ray bursts and the model of a spreading layer of accreting matter over the neutron star surface

Abstract

We report the detection during the JEM-X/INTEGRAL observations of several X-ray bursters of series of close type I X-ray bursts consisting of two or three events with a recurrence time much shorter than the characteristic (at the observed mean accretion rate) time of matter accumulation needed for a thermonuclear explosion to be initiated on the neutron star surface. We show that such series of bursts are naturally explained in the model of a spreading layer of accreting matter over the neutron star surface in the case of a sufficiently high ($\dot{M}\geq 1\times 10^{-9}\ M_{\odot}\ \mbox{yr}^{-1}$) accretion rate (corresponding to a mean luminosity $L_{\rm tot}\geq 1\times 10^{37} \mbox{erg s}^{-1}$). The existence of triple bursts requires some refinement of the model - the importance of a central ring zone is shown. In the standard model of a spreading layer no infall of matter in this zone is believed to occur.

20 pages, 5 figures

References in corpus (6)

• Thermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer
• Spread of Matter over a Neutron-Star Surface During Disk Accretion: Deceleration of Rapid Rotation
• Sedimentation and Type I X-ray Bursts at Low Accretion Rates
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• NuSTAR and AstroSat observations of thermonuclear X-ray bursts with short-recurrence times in 4U 1636$-$536