Indications for a slow rotator in the Rapid Burster from its thermonuclear bursting behaviour
arXiv:1302.4286 · doi:10.1093/mnras/stt312
Abstract
We perform time-resolved spectroscopy of all the type I bursts from the Rapid Burster (MXB 1730-335) detected with the Rossi X-ray Timing Explorer. Type I bursts are detected at high accretion rates, up to \sim 45% of the Eddington luminosity. We find evidence that bursts lacking the canonical cooling in their time-resolved spectra are, none the less, thermonuclear in nature. The type I bursting rate keeps increasing with the persistent luminosity, well above the threshold at which it is known to abruptly drop in other bursting low-mass X-ray binaries. The only other known source in which the bursting rate keeps increasing over such a large range of mass accretion rates is the 11 Hz pulsar IGR J174802446. This may indicate a similarly slow spin for the neutron star in the Rapid Burster.
References in corpus (40)
- Thermonuclear (type-I) X-ray bursts observed by the Rossi X-ray Timing Explorer
- Calibration of the Rossi X-ray Timing Explorer Proportional Counter Array
- The Ocean and Crust of a Rapidly Accreting Neutron Star: Implications for Magnetic Field Evolution and Thermonuclear Flashes
- Thermonuclear burst oscillations
- Episodic Accretion on to Strongly Magnetic Stars
- Propagation of thermonuclear flames on rapidly rotating neutron stars: extreme weather during type I X-ray bursts
- Accretion Discs Trapped Near Corotation
- Rotational Evolution During Type I X-Ray Bursts
- Evidence for "Propeller" Effects In X-ray Pulsars GX 1+4 And GROJ1744-28
- Six years of BeppoSAX Wide Field Cameras observations of nine galactic type-I X-ray bursters
- Periodic Thermonuclear X-ray Bursts from GS 1826-24 and the Fuel Composition as a Function of Accretion Rate
- A Possible Explanation for the "Parallel Tracks" Phenomenon in Low-Mass X-Ray Binaries
- Millihertz Quasi-Periodic Oscillations from Marginally Stable Nuclear Burning on an Accreting Neutron Star
- Near Infrared properties of 12 Globular Clusters toward the inner Bulge of the Galaxy
- Discovery of the Neutron Star Spin Frequency in EXO 0748-676
- Millihertz quasi-periodic oscillations and thermonuclear bursts from Terzan 5: A showcase of burning regimes
- A Fast X-ray Disk Wind in the Transient Pulsar IGR J17480-2446 in Terzan 5
- Multi-Instrument X-ray Observations of Thermonuclear Bursts with Short Recurrence Times
- A superburst from 4U 1254-690
- Eddington-limited X-ray Bursts as Distance Indicators. I. Systematic Trends and Spherical Symmetry in Bursts from 4U 1728-34
- Superburst Models for Neutron Stars with Hydrogen and Helium-Rich Atmospheres
- On the spin-up/spin-down transitions in accreting X-ray binaries
- Discovery of a 552 Hz burst oscillation in the low-mass X-ray binary EXO 0748-676
- The spin and orbit of the newly discovered pulsar IGR J17480-2446
- Discovery of X-ray burst triplets in EXO 0748-676
- The effect of rotation on the stability of nuclear burning in accreting neutron stars
- Implications of burst oscillations from the slowly rotating accreting pulsar IGR 17480-2446 in the globular cluster Terzan 5
- Why is it Difficult to Detect a Millisecond Pulsar in Neutron Star X-ray Binaries?
- Spectral and timing properties of the accreting X-ray millisecond pulsar IGR J17511-3057
- Long-Term evolution of Discs around Magnetic Stars
- The Evolution of Rapid Burster Outbursts
- The Peculiar Evolutionary History of IGR J17480-2446 in Terzan 5
- X-ray bursts and burst oscillations from the slowly spinning X-ray pulsar IGR J17480-2446 (Terzan 5)
- Is the Lack of Pulsations in Low Mass X-Ray Binaries due to Comptonizing Coronae?
- On the Nature of the Bursting X-Ray Pulsar GRO J1744-28
- On the cooling tails of thermonuclear X-ray bursts: the IGR J17480-2446 link
- Search for Millisecond Periodicities in Type I X-ray Bursts of the Rapid Burster
- A change in the outburst recurrence time of the Rapid Burster
- X-ray bursts from the Terzan 5 transient IGR J17480-2446: nuclear rather than gravitational
- The discovery of hard X-ray emission in the persistent flux of the Rapid Burster
Cited by in corpus (15)
- The Multi-INstrument Burst ARchive (MINBAR)
- Evidence for enhanced persistent emission during sub-Eddington thermonuclear bursts
- Repetitive Patterns in Rapid Optical Variations in the Nearby Black-hole Binary V404 Cygni
- The influence of accretion rate and metallicity on thermonuclear bursts: predictions from KEPLER models
- A population study of type II bursts in the Rapid Burster
- A strongly truncated inner accretion disk in the Rapid Burster
- Discovery of GRS 1915+105 variability patterns in the Rapid Burster
- Neutron star cooling and the rp process in thermonuclear X-ray bursts
- Double-peaked thermonuclear bursts at the soft-hard state transition in the Rapid Burster
- NinjaSat monitoring of Type-I X-ray bursts from the clocked burster SRGA J144459.2604207
- Disk reflection and energetics from the accreting millisecond pulsar SRGA J144459.2-604207
- New insight into the Rapid Burster by Insight-HXMT
- Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs
- A candidate to the long sought optical counterpart to the Rapid Burster in the bulge fossil fragment Liller 1
- Recurrent Instability in LMXB Accretion Disks: How Strange is GRS 1915+105?