Fast Transitions of X-ray Variability in the Neutron Star Low Mass X-ray Binary Cygnus X-2
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arXiv
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| Main Authors: | , , , , , , , , , , , , , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866918060218122240 |
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| author | Zhang, Liang Méndez, Mariano Feng, Hua Altamirano, Diego Yang, Zi-xu Zhao, Qing-chang Zhang, Shuang-nan Tao, Lian Huang, Yue Ma, Xiang Jia, Shu-mei Ge, Ming-yu Song, Li-ming Qu, Jin-lu Zhang, Shu |
| author_facet | Zhang, Liang Méndez, Mariano Feng, Hua Altamirano, Diego Yang, Zi-xu Zhao, Qing-chang Zhang, Shuang-nan Tao, Lian Huang, Yue Ma, Xiang Jia, Shu-mei Ge, Ming-yu Song, Li-ming Qu, Jin-lu Zhang, Shu |
| contents | We present a spectral-timing analysis of two NICER observations of the weakly magnetized neutron star low-mass X-ray binary Cygnus X-2. During these observations, we detect a rapid transition from a narrow 50-Hz horizontal-branch oscillation to a broad 5-Hz normal-branch oscillation, accompanied by an increase in source flux and a decrease in spectral hardness. Thanks to the large effective area of NICER, we are able to conduct a detailed comparison of the spectra associated with different types of quasi-periodic oscillations (QPOs) on short timescales. By fitting the spectra with a model that includes a disc and Comptonization components plus two emission lines, we find that the parameters of the disc component do not change significantly during the transition. However, assuming a fixed electron temperature, the optical depth of the Comptonization component decreases significantly. This drop in optical depth may be attributed to the expansion of the boundary layer or spreading layer.In addition, we find that the rms spectra for both the HBO and NBO are hard, suggesting that the boundary layer or spreading layer is driving the variability. We discuss the potential physical origin of the different types of QPOs. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2506_13503 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Fast Transitions of X-ray Variability in the Neutron Star Low Mass X-ray Binary Cygnus X-2 Zhang, Liang Méndez, Mariano Feng, Hua Altamirano, Diego Yang, Zi-xu Zhao, Qing-chang Zhang, Shuang-nan Tao, Lian Huang, Yue Ma, Xiang Jia, Shu-mei Ge, Ming-yu Song, Li-ming Qu, Jin-lu Zhang, Shu High Energy Astrophysical Phenomena We present a spectral-timing analysis of two NICER observations of the weakly magnetized neutron star low-mass X-ray binary Cygnus X-2. During these observations, we detect a rapid transition from a narrow 50-Hz horizontal-branch oscillation to a broad 5-Hz normal-branch oscillation, accompanied by an increase in source flux and a decrease in spectral hardness. Thanks to the large effective area of NICER, we are able to conduct a detailed comparison of the spectra associated with different types of quasi-periodic oscillations (QPOs) on short timescales. By fitting the spectra with a model that includes a disc and Comptonization components plus two emission lines, we find that the parameters of the disc component do not change significantly during the transition. However, assuming a fixed electron temperature, the optical depth of the Comptonization component decreases significantly. This drop in optical depth may be attributed to the expansion of the boundary layer or spreading layer.In addition, we find that the rms spectra for both the HBO and NBO are hard, suggesting that the boundary layer or spreading layer is driving the variability. We discuss the potential physical origin of the different types of QPOs. |
| title | Fast Transitions of X-ray Variability in the Neutron Star Low Mass X-ray Binary Cygnus X-2 |
| topic | High Energy Astrophysical Phenomena |
| url | https://arxiv.org/abs/2506.13503 |