NICER Observation of Unusual Burst Oscillations in 4U 1728-34
arXiv:1908.01206 · doi:10.3847/1538-4357/ab20c4
Abstract
The Neutron Star Interior Composition Explorer (NICER) has observed seven thermonuclear X-ray bursts from the Low Mass X-ray Binary (LMXB) neutron star 4U 1728-34 from the start of the mission's operations until February of 2019. Three of these bursts show oscillations in their decaying tail with frequencies that are within 1 Hz of the previously detected burst oscillations from this source. Two of these burst oscillations have unusual properties: They have large fractional rms amplitudes of and , and they are detected only at photon energies above 6 keV. By contrast, the third detected burst oscillation is compatible with previous observations of this source, with a fractional rms amplitude of rms in the 0.3 to 6.2 keV energy band. We discuss the implications of these large-amplitude burst oscillations, finding they are difficult to explain with the current theoretical models for X-ray burst tail oscillations.
arXiv comment14 pages, 6 figures, published in ApJ 878, 2, 145
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Cited by in corpus (7)
- The X-ray bursts of XTE J1739-285: a NICER sample
- Thermonuclear X-ray bursts from LMXB 4U 1636536 observed with AstroSat
- Nuclear-powered X-ray millisecond pulsars
- Discovery of a 584.65 Hz Burst Oscillation in the Low Mass X-Ray Binary 4U 1730--22
- GECAM detection of a bright type-I X-ray burst from 4U 0614+09: confirmation its spin frequency at 413 Hz
- AstroSat and NuSTAR observations of XTE J1739-285 during the 2019-2020 outburst
- A transition from mixed-fuel to pure-helium thermonuclear bursts in Terzan 5 X-3/Swift J174805.3-244637