Relativistic outflow from two thermonuclear shell flashes on neutron stars
arXiv:1407.0300 · doi:10.1051/0004-6361/201424044
Abstract
We study the exceptionally short (32-41 ms) precursors of two intermediate-duration thermonuclear X-ray bursts observed with RXTE from the neutron stars in 4U 0614+09 and 2S 0918-549. They exhibit photon fluxes that surpass those at the Eddington limit later in the burst by factors of 2.6 to 3.1. We are able to explain both the short duration and the super-Eddington flux by mildly relativistic outflow velocities of 0.1 to 0.3 subsequent to the thermonuclear shell flashes on the neutron stars. These are the highest velocities ever measured from any thermonuclear flash. The precursor rise times are also exceptionally short: about 1 ms. This is inconsistent with predictions for nuclear flames spreading laterally as deflagrations and suggests detonations instead. This is the first time that a detonation is suggested for such a shallow ignition column depth ( = 10 g cm). The detonation would possibly require a faster nuclear reaction chain, such as bypassing the alpha-capture on C with the much faster C(p,)N(,p)O process previously proposed. We confirm the possibility of a detonation, albeit only in the radial direction, through the simulation of the nuclear burning with a large nuclear network and at the appropriate ignition depth, although it remains to be seen whether the Zel'dovich criterion is met. A detonation would also provide the fast flame spreading over the surface of the neutron star to allow for the short rise times. (...) As an alternative to the detonation scenario, we speculate on the possibility that the whole neutron star surface burns almost instantly in the auto-ignition regime. This is motivated by the presence of 150 ms precursors with 30 ms rise times in some superexpansion bursts from 4U 1820-30 at low ignition column depths of ~10 g cm.
arXiv comment11 pages, 6 figures, accepted by Astronomy and Astrophysics
References in corpus (41)
- Unsteady Outflow Models for Cosmological Gamma-Ray Bursts
- 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
- Photospheric radius expansion X-ray bursts as standard candles
- Models for Type I X-Ray Bursts with Improved Nuclear Physics
- A Remarkable Three Hour Thermonuclear Burst From 4U 1820-30
- Carbon Flashes in the Heavy Element Ocean on Accreting Neutron Stars
- The Large Observatory for X-ray Timing (LOFT)
- Thermonuclear burst oscillations
- Propagation of thermonuclear flames on rapidly rotating neutron stars: extreme weather during type I X-ray bursts
- Six new candidate ultracompact X-ray binaries
- Long Type I X-ray Bursts and Neutron Star Interior Physics
- Exposing the Nuclear Burning Ashes of Radius Expansion Type I X-ray Bursts
- Evidence for accretion rate change during type I X-ray bursts
- X-ray bursting neutron star atmosphere models using an exact relativistic kinetic equation for Compton scattering
- On the possibility of a helium white dwarf donor in the presumed ultracompact binary 2S 0918-549
- Models of Type I X-Ray Bursts in 4U 1820-30
- Optical spectra of the carbon-oxygen accretion discs in the ultra-compact X-ray binaries 4U 0614+09, 4U 1543-624 and 2S 0918-549
- Models of Type I X-ray Bursts from GS 1826-24: A Probe of rp-Process Hydrogen Burning
- Ultracompact X-Ray Binaries with Neon-Rich Degenerate Donors
- Optical spectroscopy of (candidate) ultra-compact X-ray binaries: constraints on the composition of the donor stars
- Millihertz Quasi-Periodic Oscillations from Marginally Stable Nuclear Burning on an Accreting Neutron Star
- What ignites on the neutron star of 4U 0614+091?
- Evidence of heavy-element ashes in thermonuclear X-ray bursts with photospheric superexpansion
- A bright thermonuclear X-ray burst simultaneously observed with Chandra and RXTE
- X-ray emission and absorption features during an energetic thermonuclear X-ray burst from IGR J17062-6143
- Multi-Zone Models of Superbursts from Accreting Neutron Stars
- Achromatic late-time variability in thermonuclear X-ray bursts - an accretion disk disrupted by a nova-like shell?
- Flame Propagation on the Surfaces of Rapidly Rotating Neutron Stars during Type I X-ray Bursts
- Time-resolved optical photometry of the ultra-compact binary 4U0614+091
- Discovery of the Spin Frequency of 4U 0614+09 with SWIFT/BAT
- INTEGRAL detection of a long powerful burst from SLX1735-269
- Advances in the RXTE Proportional Counter Array Calibration: Nearing the Statistical Limit
- Winds from Neutron Stars and Strong Type I X--Ray Bursts
- Restless quiescence: thermonuclear flashes between transient X-ray outbursts
- BeppoSAX-WFC monitoring of the Galactic Center region
- An X-ray and optical study of the ultracompact X-ray binary A1246-58
- The Likely Orbital Period of the Ultracompact Low-Mass X-Ray Binary 2S 0918-549
- Superexpansion as a possible probe of accretion in 4U 1820-30
- The cooling rate of neutron stars after thermonuclear shell flashes
- Carbon Detonation and Shock-Triggered Helium Burning in Neutron Star Superbursts
Cited by in corpus (13)
- The Multi-INstrument Burst ARchive (MINBAR)
- Frontiers in Nuclear Astrophysics
- Thermonuclear X-ray bursts
- Nuclear Physics of the Outer Layers of Accreting Neutron Stars
- Accretion disks and coronae in the X-ray flashlight
- Observatory science with eXTP
- X-ray Reflection and An Exceptionally Long Thermonuclear Helium Burst from IGR J17062-6143
- A population study of type II bursts in the Rapid Burster
- Searching for the most powerful thermonuclear X-ray bursts with the Neil Gehrels Swift Observatory
- A catalogue of unusually long thermonuclear bursts on neutron stars
- Super-Eddington winds from Type I X-ray bursts
- Fundamental physics with neutron stars
- Mass-Radius Constraints for 2S 0918-549 from an RXTE Superexpansion Burst: A Direct Cooling-Tail Analysis