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高能物理研究所 [20]
新疆天文台 [1]
云南天文台 [1]
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期刊论文 [22]
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2021 [8]
2020 [4]
2019 [5]
2018 [4]
2017 [1]
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Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign
期刊论文
The Astrophysical Journal Letters, 2021, 卷号: 911, 期号: 1
作者:
Algaba,J. C.
;
Anczarski,J.
;
Asada,K.
;
Balokovi?,M.
;
Chandra,S.
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浏览/下载:148/0
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提交时间:2021/05/24
Active galactic nuclei
Radio cores
Low-luminosity active galactic nuclei
High energy astrophysics
Astrophysical black holes
Accretion
HXMT identification of a non-thermal X-ray burst from SGR J1935+2154 and with FRB 200428
期刊论文
Nature Astronomy, 2021, 卷号: 5, 页码: 378-384
作者:
Li, C. K.
;
Lin, L.
;
Xiong, S. L.
;
Ge, M. Y.
;
Li, X. B.
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提交时间:2021/11/18
Astrophysics - High Energy Astrophysical Phenomena
Astrophysics -
Instrumentation and Methods for Astrophysics
Detection of two bright radio bursts from magnetar SGR 1935 + 2154
期刊论文
Nature Astronomy, 2021, 卷号: 5, 页码: 414
作者:
Kirsten, F.
;
Snelders, M. P.
;
Jenkins, M.
;
Nimmo, K.
;
van den Eijnden, J.
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浏览/下载:42/0
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提交时间:2021/11/18
Astrophysics - High Energy Astrophysical Phenomena
Abstract: Fast radio bursts are millisecond-duration, bright radio signals (fluence 0.1-100 Jy ms) emitted from extragalactic sources of unknown physical origin. The recent CHIME/FRB and STARE2 detection of an extremely bright (fluence ~MJy ms) radio burst from the Galactic magnetar SGR 1935+2154 supports the hypothesis that (at least some) fast radio bursts are emitted by magnetars at cosmological distances. In follow-up observations totalling 522.7 h on source, we detect two bright radio bursts with fluences of 112 ± 22 Jy ms and 24 ± 5 Jy ms, respectively. Both bursts appear to be affected by interstellar scattering and we measure significant linear and circular polarization for the fainter burst. The bursts are separated in time by ~1.4 s, suggesting a non-Poissonian, clustered emission processsimilar to those seen in some repeating fast radio bursts. Together with the burst reported by CHIME/FRB and STARE2, as well as a much fainter burst seen by FAST (fluence 60 mJy ms), our observations demonstrate that SGR 1935+2154 can produce bursts with apparent energies spanning roughly seven orders of magnitude, and that the burst rate is comparable across this range. This raises the question of whether these four bursts arise from similar physical processes, and whether the fast radio burst population distribution extends to very low energies (~10
30
erg, isotropic equivalent).
Search for gamma-ray bursts and gravitational wave electromagnetic counterparts with High Energy X-ray Telescope of Insight-HXMT
期刊论文
Monthly Notices of the Royal Astronomical Society, 2021, 卷号: 508, 页码: 3910
作者:
Cai, C.
;
Xiong, S. L.
;
Li, C. K.
;
Liu, C. Z.
;
Zhang, S. N.
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提交时间:2021/11/18
gravitational waves
methods: observational
gamma-ray bursts
Astrophysics - High Energy Astrophysical Phenomena
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.
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浏览/下载:10/0
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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.
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浏览/下载:56/0
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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
QPOs and orbital elements of X-ray binary 4U 0115+63 during the 2017 outburst observed by Insight-HXMT
期刊论文
Monthly Notices of the Royal Astronomical Society, 2021, 卷号: 503, 页码: 6045
作者:
Ding, Y. Z.
;
Wang, W.
;
Zhang, P.
;
Bu, Q. C.
;
Cai, C.
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浏览/下载:22/0
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提交时间:2021/11/18
stars: individual: 4U 0115+63
X-rays: binaries
X-rays: stars
Astrophysics - High Energy Astrophysical Phenomena
Study on the Energy Limits of kHz QPOs in Sco X-1 with RXTE and Insight-HXMT Observations
期刊论文
The Astrophysical Journal, 2021, 卷号: 913, 页码: 119
作者:
Jia, S. M.
;
Qu, J. L.
;
Lu, F. J.
;
Zhang, S. N.
;
Zhang, S.
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浏览/下载:15/0
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提交时间:2021/11/18
X-ray binary stars
1811
Astrophysics - High Energy Astrophysical
Phenomena
Formation and Evolution of Ultraluminous X-Ray Pulsar Binaries to Pulsar-Neutron Star and Pulsar-White Dwarf Systems
期刊论文
The Astrophysical Journal, 2020, 卷号: 902, 页码: 125
作者:
Abdusalam, K.
;
Ablimit, Iminhaji
;
Hashim, P.
;
Lü, G. -L.
;
Mardini, M. K.
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浏览/下载:16/0
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提交时间:2021/06/25
Binary stars
Close binary stars
X-ray binary stars
Pulsars
Gravitational wave sources
White dwarf stars
Compact objects
154
254
1811
1306
677
1799
288
Astrophysics - High Energy
Astrophysical Phenomena
No pulsed radio emission during a bursting phase of a Galactic magnetar
期刊论文
Nature, Nature, 2020, 2020, 卷号: 587, 587, 页码: 63-65, 63-65
作者:
HXMT
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浏览/下载:4/0
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提交时间:2022/02/08
Astrophysics - High Energy Astrophysical Phenomena
Astrophysics - High Energy Astrophysical Phenomena
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