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高能物理研究所 [100]

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	Luminosity Dependence of the Cyclotron Line Energy in 1A 0535+262 Observed by Insight-HXMT during the 2020 Giant Outburst 期刊论文 The Astrophysical Journal, 2021, 卷号: 917, 页码: L38 作者: Kong, L. D.; Zhang, S.; Ji, L.; Reig, P.; Doroshenko, V. 收藏 \| 浏览/下载：10/0 \| 提交时间：2021/11/18 X-ray astronomy High mass x-ray binary stars Pulsars 1810 733 1306 Astrophysics - High Energy Astrophysical Phenomena
	Physical origin of the non-physical spin evolution of MAXI J1820 + 070 期刊论文 Monthly Notices of the Royal Astronomical Society, 2021, 卷号: 504, 页码: 2168 作者: Guan, J.; Tao, L.; Qu, J. L.; Zhang, S. N.; Zhang, W. 收藏 \| 浏览/下载：55/0 \| 提交时间：2021/11/18 accretion accretion discs black hole physics stars: individual (MAXI J1820 + 070) X-rays: binaries Astrophysics - High Energy Astrophysical Phenomena 83C57
	The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition 期刊论文 Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 494, 页码: 1865-1870 作者: HXMT 收藏 \| 浏览/下载：15/0 \| 提交时间：2022/02/08 stars: magnetic field stars: neutron pulsars: general Astrophysics - High Energy Astrophysical Phenomena
	Insight-HXMT observations of Swift J0243.6+6124: the evolution of RMS pulse fractions at super-Eddington luminosity 期刊论文 Monthly Notices of the Royal Astronomical Society, 2020, 卷号: 497, 页码: 5498-5506 作者: HXMT 收藏 \| 浏览/下载：11/0 \| 提交时间：2022/02/08 stars: neutron pulsars: individual: Swift J0243.6+6124 X-rays: binaries
	Long-term evolutions of the cyclotron line energies in her x-1, vela x-1, and cen x-3 as observed with swift/bat 期刊论文 Monthly notices of the royal astronomical society, 2019, 卷号: 484, 期号: 3, 页码: 3797-3805 作者: Ji, L.; Staubert, R.; Ducci, L.; Santangelo, A.; Zhang, S. 收藏 \| 浏览/下载：64/0 \| 提交时间：2019/04/22 Radiation mechanisms: thermal Scattering Stars: magnetic field Stars: neutron X-rays: binaries X-rays: individual: her x-1, vela x-1, cen x-3
	Long-term evolutions of the cyclotron line energies in her x-1, vela x-1, and cen x-3 as observed with swift/bat 期刊论文 Monthly notices of the royal astronomical society, 2019, 卷号: 484, 期号: 3, 页码: 3797-3805 作者: Ji, L.; Staubert, R.; Ducci, L.; Santangelo, A.; Zhang, S. 收藏 \| 浏览/下载：64/0 \| 提交时间：2019/04/22 Radiation mechanisms: thermal Scattering Stars: magnetic field Stars: neutron X-rays: binaries X-rays: individual: her x-1, vela x-1, cen x-3
	Unifying neutron star sub-populations in the supernova fallback accretion model 期刊论文 Research in astronomy and astrophysics, 2019, 卷号: 19, 期号: 3, 页码: 12 作者: Liu, Bai-Sheng; Li, Xiang-Dong 收藏 \| 浏览/下载：179/0 \| 提交时间：2019/04/22 Accretion, accretion disks Stars: neutron, evolution, rotation, magnetic field, magnetars Pulsars: general
	Unifying neutron star sub-populations in the supernova fallback accretion model 期刊论文 Research in astronomy and astrophysics, 2019, 卷号: 19, 期号: 3, 页码: 12 作者: Liu, Bai-Sheng; Li, Xiang-Dong 收藏 \| 浏览/下载：179/0 \| 提交时间：2019/04/22 Accretion, accretion disks Stars: neutron, evolution, rotation, magnetic field, magnetars Pulsars: general
	Insight-HXMT Observations of Swift J0243.6+6124 during Its 20172018 Outburst 期刊论文 The Astrophysical Journal, 2019, 卷号: 879 作者: Zhang, Wei; Zhang, WanChang; Zhang, WenZhao; Zhang, Yi; Zhang, YiFei 收藏 \| 浏览/下载：187/0 \| 提交时间：2019/07/12 accretion accretion disks pulsars: individual: Swift J0243.6+6124 stars: distances stars: magnetic field X-rays: binaries Astrophysics - High Energy Astrophysical Phenomena
	Constant cyclotron line energy in Hercules X-1 - Joint Insight-HXMT and NuSTAR observations 期刊论文 Journal of High Energy Astrophysics, 2019, 卷号: 23, 页码: 29-32 作者: HXMT 收藏 \| 浏览/下载：33/0 \| 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.

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