NICER, NuSTAR, and Insight-HXMT Views to the Newly Discovered Black Hole X-Ray Binary Swift J1727.8-1613

Swift J1727.8–1613 is a black hole X-ray binary newly discovered in 2023. We perform spectral analysis with simultaneous Insight-HXMT, NICER, and NuSTAR observations when the source was approaching the hard intermediate state. Such a joint view reveals an additional hard component apart from the nor...

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Published inAstrophysical journal. Letters Vol. 960; no. 2; p. L17
Main Authors Peng, Jing-Qiang, Zhang, Shu, Shui, Qing-Cang, Zhang, Shuang-Nan, Kong, Ling-Da, Chen, Yu-Peng, Wang, Peng-Ju, Ji, Long, Qu, Jin-Lu, Tao, Lian, Ge, Ming-Yu, Chang, Zhi, Li, Jian, Li, Zhao-sheng, Yu, Zhuo-Li, Yan, Zhe
Format Journal Article
LanguageEnglish
Published Austin The American Astronomical Society 01.01.2024
IOP Publishing
Subjects
Black holes
Corona
Spectral analysis
Spectrum analysis
X ray binaries
X ray stars
X-ray astronomy
X-ray binary stars
X-rays
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Abstract Swift J1727.8–1613 is a black hole X-ray binary newly discovered in 2023. We perform spectral analysis with simultaneous Insight-HXMT, NICER, and NuSTAR observations when the source was approaching the hard intermediate state. Such a joint view reveals an additional hard component apart from the normally observed hard component with reflection in the spectrum, to be distinguished from the usual black hole X-ray binary systems. By including this extra component in the spectrum, we have measured a high spin of 0.98 − 0.07 + 0.02 and an inclination of around 40 − 0.8 + 1.2 °, which is consistent with NICER results reported before. However, we find that the additional spectral component cannot be exclusively determined due to the model degeneracy. Accordingly, a possible jet/corona configuration is adjusted to account for the spectral fitting with different model trials. The extra component may originate either from a relativistic jet or a jet base/corona underneath a slow jet.
AbstractList Swift J1727.8–1613 is a black hole X-ray binary newly discovered in 2023. We perform spectral analysis with simultaneous Insight-HXMT, NICER, and NuSTAR observations when the source was approaching the hard intermediate state. Such a joint view reveals an additional hard component apart from the normally observed hard component with reflection in the spectrum, to be distinguished from the usual black hole X-ray binary systems. By including this extra component in the spectrum, we have measured a high spin of ${0.98}_{-0.07}^{+0.02}$ and an inclination of around ${40}_{-0.8}^{+1.2}$ °, which is consistent with NICER results reported before. However, we find that the additional spectral component cannot be exclusively determined due to the model degeneracy. Accordingly, a possible jet/corona configuration is adjusted to account for the spectral fitting with different model trials. The extra component may originate either from a relativistic jet or a jet base/corona underneath a slow jet.
Swift J1727.8–1613 is a black hole X-ray binary newly discovered in 2023. We perform spectral analysis with simultaneous Insight-HXMT, NICER, and NuSTAR observations when the source was approaching the hard intermediate state. Such a joint view reveals an additional hard component apart from the normally observed hard component with reflection in the spectrum, to be distinguished from the usual black hole X-ray binary systems. By including this extra component in the spectrum, we have measured a high spin of 0.98−0.07+0.02 and an inclination of around 40−0.8+1.2°, which is consistent with NICER results reported before. However, we find that the additional spectral component cannot be exclusively determined due to the model degeneracy. Accordingly, a possible jet/corona configuration is adjusted to account for the spectral fitting with different model trials. The extra component may originate either from a relativistic jet or a jet base/corona underneath a slow jet.
Swift J1727.8–1613 is a black hole X-ray binary newly discovered in 2023. We perform spectral analysis with simultaneous Insight-HXMT, NICER, and NuSTAR observations when the source was approaching the hard intermediate state. Such a joint view reveals an additional hard component apart from the normally observed hard component with reflection in the spectrum, to be distinguished from the usual black hole X-ray binary systems. By including this extra component in the spectrum, we have measured a high spin of 0.98 − 0.07 + 0.02 and an inclination of around 40 − 0.8 + 1.2 °, which is consistent with NICER results reported before. However, we find that the additional spectral component cannot be exclusively determined due to the model degeneracy. Accordingly, a possible jet/corona configuration is adjusted to account for the spectral fitting with different model trials. The extra component may originate either from a relativistic jet or a jet base/corona underneath a slow jet.
Author Qu, Jin-Lu
Li, Zhao-sheng
Kong, Ling-Da
Chen, Yu-Peng
Peng, Jing-Qiang
Wang, Peng-Ju
Yan, Zhe
Ji, Long
Shui, Qing-Cang
Zhang, Shuang-Nan
Tao, Lian
Chang, Zhi
Ge, Ming-Yu
Yu, Zhuo-Li
Zhang, Shu
Li, Jian
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Snippet Swift J1727.8–1613 is a black hole X-ray binary newly discovered in 2023. We perform spectral analysis with simultaneous Insight-HXMT, NICER, and NuSTAR...
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StartPage L17
SubjectTerms Black holes
Corona
Spectral analysis
Spectrum analysis
X ray binaries
X ray stars
X-ray astronomy
X-ray binary stars
X-rays
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Title NICER, NuSTAR, and Insight-HXMT Views to the Newly Discovered Black Hole X-Ray Binary Swift J1727.8-1613
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