XMM-Newton and NICER measurement of the rms spectrum of the millihertz quasi-periodic oscillations in the neutron-star low-mass X-ray binary 4U 1636-53
arXiv:2006.09563 · doi:10.3847/1538-4357/ab8cbe
Abstract
We used two XMM-Newton and six Neutron Star Interior Composition Explorer (NICER) observations to investigate the fractional rms amplitude of the millihertz quasi-periodic oscillations (mHz QPOs) in the neutron-star low-mass X-ray binary 4U 1636-53. We studied, for the first time, the fractional rms amplitude of the mHz QPOs vs. energy in 4U 1636-53 down to 0.2 keV. We find that, as the energy increases from 0.2 keV to 3 keV, the rms amplitude of the mHz QPOs increases, different from the decreasing trend that has been previously observed above 3 keV. This finding has not yet been predicted by any current theoretical model, however, it provides an important observational feature to speculate whether a newly discovered mHz oscillation originates from the marginally stable nuclear burning process on the neutron star surface.
arXiv commentPublished in ApJ, 10 pages, 5 figures
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Cited by in corpus (5)
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- Detection of millihertz quasi-periodic oscillations in the low-mass X-ray binary 4U 1730--22 with NICER
- Drifts of the marginally stable burning frequency in the X-ray binaries 4U 1608--52 and Aql X--1
- The harmonic component of the millihertz quasi-periodic oscillations in 4U 1636-53
- The mHz quasi-regular modulations of 4U 1630--47 during its 1998 outburst