A Strong X-Ray Burst from the Low Mass X-Ray Binary EXO0748-676
arXiv:astro-ph/0506515 · doi:10.1086/444348
Abstract
We have observed an unusually strong X-ray burst as a part of our regular eclipse timing observations of the low mass binary system EXO0748-676. The burst peak flux was 5.2x10^-8 ergs cm^-2 s^-1, approximately five times the normal peak X-ray burst flux observed from this source by RXTE. Spectral fits to the data strongly suggest that photospheric radius expansion occurred during the burst. In this Letter we examine the properties of this X-ray burst, which is the first example of a radius expansion burst from EXO0748-676 observed by RXTE. We find no evidence for coherent burst oscillations. Assuming that the peak burst luminosity is the Eddington luminosity for a 1.4 solar mass neutron star we derive a distance to EXO0748-676 of 7.7 kpc for a helium-dominated burst photosphere and 5.9 kpc for a hydrogen-dominated burst photosphere.
15 pages including 2 figures and 1 table. Accepted for publication in the Astrophysical Journal
References in corpus (9)
- Neutron Star Structure and the Equation of State
- Gravitationally redshifted absorption lines in the X-ray burst spectra of a neutron star
- Photospheric radius expansion X-ray bursts as standard candles
- The distances to Galactic low-mass X-ray binaries: consequences for black hole luminosities and kicks
- A Remarkable Three Hour Thermonuclear Burst From 4U 1820-30
- Recent Progress in Neutron Star Theory
- Discovery of the Neutron Star Spin Frequency in EXO 0748-676
- Eddington-limited X-ray Bursts as Distance Indicators. I. Systematic Trends and Spherical Symmetry in Bursts from 4U 1728-34
- A Second Intense Burst with Photospheric Radius Expansion from X2127+119 in M15
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- Biases for neutron-star mass, radius and distance measurements from Eddington-limited X-ray bursts
- Discovery of X-ray burst triplets in EXO 0748-676
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- Discovery of millihertz quasi-periodic oscillations in the X-ray binary EXO 0748--676
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- Suzaku Observation of the High-Inclination Binary EXO 0748-676 in the Hard State
- RXTE/ASM and Swift/BAT Observations of Spectral Transitions in Bright X-ray Binaries in 2005-2010
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- Astrophysics in 2006
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