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	Repeating X-ray bursts: Interaction between a neutron star and clumps partially disrupted from a planet 期刊论文 OAI收割 ASTRONOMY & ASTROPHYSICS, 2024, 卷号: 686, 页码: A87 作者: Kurban, Abdusattar; Zhou, Xia; Wang, Na; Huang, Yong-Feng; Wang, Yu-Bin \| 收藏 \| 浏览/下载：2/0 \| 提交时间：2024/07/09 planet-star interactions stars: neutron X-rays: bursts
	EOS-dependent millihertz quasi-periodic oscillation in low-mass X-ray binary 期刊论文 OAI收割 MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 卷号: 525, 期号: 2, 页码: 2054-2068 作者: Liu, Helei; Gao, Yong; Li, Zhaosheng; Dohi, Akira; Wang, Weiyang \| 收藏 \| 浏览/下载：29/0 \| 提交时间：2023/11/14 accretion stars:neutron star X-rays: burst
	High plasma cut-off frequency blocks the radio emission from accreting millisecond X-ray pulsar SAX J1808.4-3658 期刊论文 OAI收割 Astrophysics and Space Science, 2020, 卷号: 365, 期号: 3, 页码: 47 作者: Wang, S. Q.; Zhang, C. M.; Wang, D. H.; Wang, N.; Wang, J. B. \| 收藏 \| 浏览/下载：26/0 \| 提交时间：2021/04/12 (Stars:) pulsar: individual: SAX J1808.4-3658 Stars neutron X-rays stars X-rays binaries X-rays: general neutron-star magnetic-field optical counterpart xmm-newton binary evolution constraints transient sax-j1808.4-3658 oscillations Astronomy & Astrophysics
	Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations 期刊论文 OAI收割 JOURNAL OF HIGH ENERGY ASTROPHYSICS, 2019, 卷号: 23, 页码: 29-32 作者: Xiao, G. C.; Ji, L.; Staubert, R.; Ge, M. Y.; Zhang, S. \| 收藏 \| 浏览/下载：14/0 \| 提交时间：2020/03/10 Stars: neutron star Pulsars: binary(Her X-1) X-rays: stars
	Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations 期刊论文 OAI收割 Journal of High Energy Astrophysics, 2019, 卷号: 23, 页码: 29-32 作者: HXMT \| 收藏 \| 浏览/下载：57/0 \| 提交时间：2022/02/08 Stars: neutron star Pulsars: binary(Her X-1) X-rays: stars Astrophysics - High Energy Astrophysical Phenomena Abstract: The long-term evolution of the centroid energy of the CRSF in Her X-1 is still a mystery. We report a new measurement from a campaign between Insight-HXMT and NuSTAR performed in February 2018. Generally, the two satellites show well consistent results of timing and spectral properties. The joint spectral analysis confirms that the previously observed long decay phase has ended, and that the line energy instead keeps constant around 37.5 keV after flux correction.
	Timing analysis of Swift J1658.2-4242's outburst in 2018 with Insight-HXMT, NICER and AstroSat 期刊论文 OAI收割 Journal of High Energy Astrophysics, 2019, 卷号: 24, 页码: 30-40 作者: HXMT \| 收藏 \| 浏览/下载：61/0 \| 提交时间：2022/02/08 Accretion accretion disks Black hole physics X-rays: binaries: Swift J1658.2-4242 Astrophysics - High Energy Astrophysical Phenomena Abstract: We present the observational results from a detailed timing analysis of the black hole candidate Swift J1658.2-4242 during its 2018 outburst with the observations of Hard X-ray Modulation Telescope (Insight-HXMT), Neutron Star Interior Composition Explorer (NICER) and AstroSat in 0.1-250 keV. The evolution of intensity, hardness and integrated fractional root mean square (rms) observed by Insight-HXMT and NICER are presented in this paper. Type-C quasi-periodic oscillations (QPOs) observed by NICER (0.8-3.5 Hz) and Insight-HXMT (1-1.6 Hz) are also reported in this work. The features of the QPOs are analyzed with an energy range of 0.5-50 keV. The relations between QPO frequency and other characteristics such as intensity, hardness and QPO rms are carefully studied. The timing and spectral properties indicate that Swift J1658.2-4242 is a black hole binary system. Besides, the rms spectra of the source calculated from the simultaneous observation of Insight-HXMT, NICER and AstroSat support the Lense-Thirring origin of the QPOs. The relation between QPO phase lag and the centroid frequency of Swift J1658.2-4242 reveals a near zero constant when < 4Hz and a soft phase lag at 6.68 Hz. This independence follows the same trend as the high inclination galactic black hole binaries such as MAXI J1659-152.
	Type-I bursts within outbursts of IGR J17473-2721 期刊论文 OAI收割 ASTRONOMY & ASTROPHYSICS, 2010, 卷号: 510, 页码: A81 作者: Chen YP(陈玉鹏); Zhang S(张澍); Wang JM(王建民); Li TB(李惕碚); Chen, YP 收藏 \| 浏览/下载：26/0 \| 提交时间：2016/06/29 star: neutron individual: IGR J17473-2721 X-rays: bursts
	The nature of AX J0051-733 in the SMC: A pulsar born with ultrastrong magnetic field? 期刊论文 OAI收割 ASTROPHYSICS AND SPACE SCIENCE, 2006, 卷号: 305, 期号: 2, 页码: 133-138 作者: Liu, Q. Z. 收藏 \| 浏览/下载：21/0 \| 提交时间：2012/02/07 binaries close-pulsars individual AX J0051-733-stars neutron star-X-rays stars-stars emission-line, Be