Probing the effects of a thermonuclear X-ray burst on the neutron star accretion flow with NuSTAR
arXiv:1601.01680 · doi:10.1093/mnras/stv2965
Abstract
Observational evidence has been accumulating that thermonuclear X-ray bursts ignited on the surface of neutron stars influence the surrounding accretion flow. Here, we exploit the excellent sensitivity of NuSTAR up to 79 keV to analyze the impact of an X-ray burst on the accretion emission of the neutron star LMXB 4U 1608-52. The ~200 s long X-ray burst occurred during a hard X-ray spectral state, and had a peak intensity of ~30-50 per cent of the Eddington limit with no signs of photospheric radius expansion. Spectral analysis suggests that the accretion emission was enhanced up to a factor of ~5 during the X-ray burst. We also applied a linear unsupervised decomposition method, namely non-negative matrix factorization (NMF), to study this X-ray burst. We find that the NMF performs well in characterizing the evolution of the burst emission and is a promising technique to study changes in the underlying accretion emission in more detail than is possible through conventional spectral fitting. For the burst of 4U 1608-52, the NMF suggests a possible softening of the accretion spectrum during the X-ray burst, which could potentially be ascribed to cooling of a corona. Finally, we report a small (~3 per cent) but significant rise in the accretion emission ~0.5 h before the X-ray burst, although it is unclear whether this was related to the X-ray burst ignition.
10 pages, 10 figures, 1 table, to appear in MNRAS
References in corpus (17)
- Thermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer
- Black hole-like hysteresis and accretion states in neutron star low mass X-ray binaries
- X-ray binaries
- The effect of accretion on the measurement of neutron star mass and radius in the low-mass X-ray binary 4U 1608-52
- Evidence for enhanced persistent emission during sub-Eddington thermonuclear bursts
- Sedimentation and Type I X-ray Bursts at Low Accretion Rates
- Analysing the atolls: X-ray spectral transitions of accreting neutron stars
- The influence of accretion geometry on the spectral evolution during thermonuclear (type-I) X-ray bursts
- First superburst from a classical low-mass X-ray binary transient
- New Constraints on the Black Hole Low/Hard State Inner Accretion Flow with NuSTAR
- Revealing the X-ray Variability of AGN with Principal Component Analysis
- X-Raying an Accretion Disk in Realtime: the Evolution of Ionized Reflection during a Superburst from 4U 1636-536
- NuSTAR observation of a Type I X-ray burst from GRS 1741.9-2853
- Characterizing the Evolving X-Ray Spectral Features During a Superburst from 4U 1636-536
- A state-dependent influence of the type-I bursts on the accretion in 4U 1608--52?
- Diagnosing the burst influence upon accretion in the clocked burster GS 1826--238
- Unsupervised spectral decomposition of X-ray binaries with application to GX 339-4
Cited by in corpus (26)
- Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
- Accretion disks and coronae in the X-ray flashlight
- Gravitational Lensing of Rays through the Levitating Atmospheres of Compact Objects
- X-ray burst induced spectral variability in 4U 1728-34
- Accretion heated atmospheres of X-ray bursting neutron stars
- NuSTAR view of the Z-type neutron star low-mass X-ray binary Cygnus~X--2
- Thermonuclear X-ray bursts in rapid succession in 4U 1636-536 with AstroSat-LAXPC
- Burst-induced coronal cooling in GS 1826-24 The clock wagging its tail
- A broadband look of the Accreting Millisecond X-ray Pulsar SAX J1748.9-2021 using AstroSat and XMM-Newton
- A catalogue of unusually long thermonuclear bursts on neutron stars
- On the disc reflection spectroscopy of NS LMXB Serpens~X-1: analysis of a recent NuSTAR observation
- NICER views moderate, strong, and extreme photospheric expansion bursts from the ultracompact X-ray binary 4U 182030
- Variable spreading layer in 4U 1608-52 during thermonuclear X-ray bursts in the soft state
- Cooling of Accretion Disc Coronae by Type I X-ray Bursts
- Accretion disk signatures in Type I X-ray Bursts: prospects for future missions
- Study of the reflection spectrum of the bright atoll source GX 3+1 with NuSTAR
- Evidence of spreading layer emission in thermonuclear superbursts
- The study of thermonuclear X-ray bursts in accreting millisecond pulsar MAXI J1816-195 with NuSTAR and NICER
- A catalog of intermediate duration Type I X-ray bursts observed with the INTEGRAL satellite
- Insight-HXMT observations on thermonuclear X-ray bursts from 4U~1608--52 in the low/hard state: the energy-dependant hard X-ray deficit and cooling saturation of the corona
- AstroSat observation of rapid Type-I thermonuclear burst from the low mass X-ray binary GX 3+1
- Detection of the thermonuclear X-ray bursts and dips from the X-ray binary 4U 1323-62 with AstroSat/LAXPC
- Thermonuclear Type-I X-ray Bursts and Burst Oscillations from the Eclipsing AMXP Swift J1749.4-2807
- The X-ray bursts within the 2010 outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021
- Resolving SLX 1744-299 and SLX 1744-300 in the hard X-ray band: implications for their ultracompact nature
- NuSTAR and AstroSat observations of thermonuclear X-ray bursts with short-recurrence times in 4U 1636536