Timing and spectral studies of the Be/X-ray binary EXO 2030+375 using Insight-HXMT observations
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| Main Authors: | , , , , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866910017988329472 |
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| author | Du, Yu-Jia Ducci, Lorenzo Ji, Long Bu, Qing-Cui Kong, Ling-Da Wang, Peng-Ju Tuo, Youli Santangelo, Andrea |
| author_facet | Du, Yu-Jia Ducci, Lorenzo Ji, Long Bu, Qing-Cui Kong, Ling-Da Wang, Peng-Ju Tuo, Youli Santangelo, Andrea |
| contents | We report the X-ray spectral and timing analysis of the high mass X-ray binary EXO 2030+375 during the 2021 type-II outburst based on the Insight-HXMT observations. Pulsations can be detected in the energy band of 1-150 keV. The pulse profile shows energy and luminosity dependence and variability. We observed transitions in the pulse profile shape during the rising and the decaying phase of the outburst. The pulse fraction exhibits an anti-correlation with luminosity and a non-monotonic energy dependence, with a possible dip near 30 keV during the outburst peak. The hardness-intensity diagrams (7-10 keV/4-7 keV) suggest state transitions during the early and late phases of the outburst. These transitions are consistent with the luminosity at which the pulse profile shape changes occur, revealing the source reaching the critical luminosity and transitioning between super-critical and sub-critical accretion regimes. We performed the average and phase-resolved spectral analysis, where the flux-resolved average spectra show a stable spectral evolution with luminosity. The phase-resolved spectral analysis reveals that the dependence of spectral parameters on the pulse phase varies with different luminosities. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2501_06013 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Timing and spectral studies of the Be/X-ray binary EXO 2030+375 using Insight-HXMT observations Du, Yu-Jia Ducci, Lorenzo Ji, Long Bu, Qing-Cui Kong, Ling-Da Wang, Peng-Ju Tuo, Youli Santangelo, Andrea High Energy Astrophysical Phenomena We report the X-ray spectral and timing analysis of the high mass X-ray binary EXO 2030+375 during the 2021 type-II outburst based on the Insight-HXMT observations. Pulsations can be detected in the energy band of 1-150 keV. The pulse profile shows energy and luminosity dependence and variability. We observed transitions in the pulse profile shape during the rising and the decaying phase of the outburst. The pulse fraction exhibits an anti-correlation with luminosity and a non-monotonic energy dependence, with a possible dip near 30 keV during the outburst peak. The hardness-intensity diagrams (7-10 keV/4-7 keV) suggest state transitions during the early and late phases of the outburst. These transitions are consistent with the luminosity at which the pulse profile shape changes occur, revealing the source reaching the critical luminosity and transitioning between super-critical and sub-critical accretion regimes. We performed the average and phase-resolved spectral analysis, where the flux-resolved average spectra show a stable spectral evolution with luminosity. The phase-resolved spectral analysis reveals that the dependence of spectral parameters on the pulse phase varies with different luminosities. |
| title | Timing and spectral studies of the Be/X-ray binary EXO 2030+375 using Insight-HXMT observations |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2501.06013 |