NICER views moderate, strong, and extreme photospheric expansion bursts from the ultracompact X-ray binary 4U 182030
arXiv:2312.16420 · doi:10.1051/0004-6361/202348195
Abstract
Type I X-ray bursts in the ultracompact X-ray binary 4U 182030 are powered by the unstable thermonuclear burning of hydrogen-deficient material. We report the detection of 15 type I X-ray bursts from 4U 182030 observed by NICER in between 2017 and 2023. All these bursts occurred in the low state for the persistent flux in the range of in 0.1250 keV. The burst spectra during the tail can be well explained by blackbody model. However, for the first 5 s after the burst onset, the time-resolved spectra showed strong deviations from the blackbody model. The significant improvement of the fit can be obtained by taking into account of the enhanced persistent emission due to the Poynting-Robterson drag, the extra emission modelled by another blackbody component or by the reflection from the surrounding accretion disk. The reflection model provides a self-consistent and physically motivated explanation. We find that the accretion disk density changed with 0.5 s delay as response to the burst radiation, which indicates the distortion of the accretion disk during X-ray bursts. From the time-resolved spectroscopy, all bursts showed the characteristic of photospheric radius expansion (PRE). We find one superexpansion burst with the extreme photospheric radius km and blackbody temperature of keV, thirteen strong PRE bursts for km, and one moderate PRE burst for km.
arXiv comment16 pages, 13 figures, 4 tables. It matches the published version in Astronomy & Astrophysics
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Cited by in corpus (9)
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