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Progress in multi-messenger observations and emission models of blazars
期刊论文
NEW ASTRONOMY REVIEWS, 2024, 卷号: 98
作者:
Cao, Gang
;
Geng, Xiongfei
;
Wang JC(王建成)
;
Yang, Xiongbang
收藏
  |  
浏览/下载:15/0
  |  
提交时间:2024/03/29
Blazars
Multi-wavelength astronomy
High energy
Neutrino astrophysics
Measurements of All-Particle Energy Spectrum and Mean Logarithmic Mass of Cosmic Rays from 0.3 to 30 PeV with LHAASO-KM2A
期刊论文
Physical Review Letters, 2024, 卷号: 132, 期号: 13
作者:
Cao, Zhen
;
Aharonian, F.
;
Axikegu
;
Bai, Y. X.
;
Bao, Y. W.
收藏
  |  
浏览/下载:21/0
  |  
提交时间:2024/04/08
Research Areas
Cosmic ray composition & spectra
Gravitation, Cosmology & Astrophysics
Uncertainties in Atomic Data for Modeling Astrophysical Charge Exchange Plasmas
期刊论文
SENSORS, 2022, 卷号: 22, 期号: 3, 页码: 13
作者:
Gu, Liyi
;
Shah, Chintan
;
Zhang, Ruitian
收藏
  |  
浏览/下载:17/0
  |  
提交时间:2022/04/11
charge exchange
X-ray astrophysics
atomic data
plasma diagnostics
First result from the Jinping Underground Nuclear Astrophysics experiment JUNA: precise measurement of the 92 keV Mg-25(p, y)Al-26 resonance
期刊论文
SCIENCE BULLETIN, 2022, 卷号: 67, 期号: 2, 页码: 125-132
作者:
Su, Jun
;
Zhang, Hao
;
Li, Zhihong
;
Ventura, Paolo
;
Li, Yunju
收藏
  |  
浏览/下载:38/0
  |  
提交时间:2022/04/11
Nuclear astrophysics
Underground laboratory
Cosmic y ray
Resonance reaction
Spectropolarimetry and photometry of the early afterglow of the gamma-ray burst GRB 191221B
期刊论文
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2021, 卷号: 506, 期号: 3, 页码: 4621-4631
作者:
Buckley, D A H
;
Bagnulo, S
;
Britto, R J
;
Mao JR(毛基荣)
;
Kann, D A
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浏览/下载:56/0
  |  
提交时间:2022/01/24
magnetic fields
gamma-ray bursts
high energy astrophysics
polarimetry
shocks
jets
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:157/0
  |  
提交时间:2021/05/24
Active galactic nuclei
Radio cores
Low-luminosity active galactic nuclei
High energy astrophysics
Astrophysical black holes
Accretion
First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon
期刊论文
ASTROPHYSICAL JOURNAL LETTERS, 2021, 卷号: 910, 期号: 1
作者:
Akiyama, Kazunori
;
Algaba, Juan Carlos
;
Alberdi, Antxon
;
Alef, Walter
;
Anantua, Richard
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  |  
浏览/下载:96/0
  |  
提交时间:2021/04/19
Accretion
Black holes
Event horizons
Jets
Kerr black holes
Magnetic fields
Magnetohydrodynamics
Plasma astrophysics
Polarimetry
Radiative transfer
Radio jets
Relativistic jets
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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  |  
浏览/下载:69/0
  |  
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:46/0
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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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浏览/下载:34/0
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提交时间:2021/11/18
gravitational waves
methods: observational
gamma-ray bursts
Astrophysics - High Energy Astrophysical Phenomena
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