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浏览/检索结果: 共17条,第1-10条 帮助

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Prospective study on observations of γ-ray sources in the Galaxy using the HADAR experiment 期刊论文  OAI收割
Frontiers of Physics, 2022, 卷号: 17, 期号: 6, 页码: 64602
作者:  
Qian, Xiangli;  Sun, Huiying;  Chen, Tianlu;  Danzengluobu;  Feng, Youliang
  |  收藏  |  浏览/下载:24/0  |  提交时间:2023/11/10
Jet Properties of Compact Steep-spectrum Sources and an Eddington-ratio-driven Unification Scheme of Jet Radiation in Active Galactic Nuclei 期刊论文  OAI收割
The Astrophysical Journal, 2020, 卷号: 899, 期号: 1
作者:  
Zhang,Jin;  Zhang,Hai-Ming;  Gan,Ying-Ying;  Yi,Ting-Feng;  Wang,Jun-Feng
  |  收藏  |  浏览/下载:32/0  |  提交时间:2021/12/06
Hadronic versus Leptonic Models for γ-Ray Emission from VER J2227+608 期刊论文  OAI收割
The Astrophysical Journal Letters, 2020, 卷号: 897, 期号: 2
作者:  
Liu,Siming;  Zeng,Houdun;  Xin,Yuliang;  Zhu,Hui
  |  收藏  |  浏览/下载:17/0  |  提交时间:2021/12/06
A Large Population of Obscured AGN in Disguise as Low-luminosity AGN in Chandra Deep Field South 期刊论文  OAI收割
The Astrophysical Journal, 2020, 卷号: 897, 期号: 2
作者:  
Lambrides,Erini L.;  Chiaberge,Marco;  Heckman,Timothy;  Gilli,Roberto;  Vito,Fabio
  |  收藏  |  浏览/下载:13/0  |  提交时间:2021/12/06
Leptonic or Hadronic Emission: The X-Ray Radiation Mechanism of Large-scale Jet Knots in 3C 273 期刊论文  OAI收割
ASTROPHYSICAL JOURNAL, 2020, 卷号: 893, 期号: 1, 页码: 11
作者:  
Wang, Zhen-Jie;  Zhang, Jin;  Sun, Xiao-Na;  Liang, En-Wei
  |  收藏  |  浏览/下载:19/0  |  提交时间:2021/12/06
An Extreme X-Ray Variability Event of a Weak-line Quasar 期刊论文  OAI收割
The Astrophysical Journal Letters, 2020, 卷号: 889, 期号: 2
作者:  
Ni,Q.;  Brandt,W. N.;  Yi,W.;  Luo,B.;  Timlin,J. D.
  |  收藏  |  浏览/下载:24/0  |  提交时间:2021/09/26
The GBT Diffuse Ionized Gas Survey: Tracing the Diffuse Ionized Gas around the Giant Hii Region W43 期刊论文  OAI收割
The Astrophysical Journal, 2020, 卷号: 889, 期号: 2
作者:  
Luisi,Matteo;  Anderson,L. D.;  Liu,Bin;  Balser,Dana S.;  Bania,T. M.
  |  收藏  |  浏览/下载:29/0  |  提交时间:2020/03/10
The Giant Radio Array for Neutrino Detection (GRAND): Science and design 期刊论文  OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2020, 卷号: 63, 期号: 1, 页码: 43
作者:  
Alvarez-Muniz, Jaime;  Batista, Rafael Alves;  Balagopal, Aswathi, V;  Bolmont, Julien;  Bustamante, Mauricio
  |  收藏  |  浏览/下载:28/0  |  提交时间:2021/09/26
Three body first post-Newtonian effects on the secular dynamics of a compact binary near a spinning supermassive black hole 期刊论文  OAI收割
PHYSICAL REVIEW D, 2020, 卷号: 102, 期号: 10, 页码: 104002
作者:  
Fang, Yun;  Huang, Qing-Guo
  |  收藏  |  浏览/下载:27/0  |  提交时间:2021/09/27
No pulsed radio emission during a bursting phase of a Galactic magnetar 期刊论文  OAI收割
Nature, 2020, 卷号: 587, 页码: 63-65
作者:  
HXMT
  |  收藏  |  浏览/下载:44/0  |  提交时间:2022/02/08
Astrophysics - High Energy Astrophysical Phenomena  Abstract: Fast radio bursts (FRBs) are millisecond-duration radio transients of unknown physical origin observed at extragalactic distances1-3. It has long been speculated that magnetars are the engine powering repeating bursts from FRB sources4-13, but no convincing evidence has been collected so far14. Recently, the Galactic magnetar SRG 1935+2154 entered an active phase by emitting intense soft íray bursts15. One FRB-like event with two peaks (FRB 200428) and a luminosity slightly lower than the faintest extragalactic FRBs was detected from the source, in association with a soft íray/hard-X-ray flare18-21. Here we report an eight-hour targeted radio observational campaign comprising four sessions and assisted by multi-wavelength (optical and hard-X-ray) data. During the third session, 29 soft-íray repeater (SGR) bursts were detected in íray energies. Throughout the observing period, we detected no single dispersed pulsed emission coincident with the arrivals of SGR bursts, but unfortunately we were not observing when the FRB was detected. The non-detection places a fluence upper limit that is eight orders of magnitude lower than the fluence of FRB 200428. Our results suggest that FRB-SGR burst associations are rare. FRBs may be highly relativistic and geometrically beamed, or FRB-like events associated with SGR bursts may have narrow spectra and characteristic frequencies outside the observed band. It is also possible that the physical conditions required to achieve coherent radiation in SGR bursts are difficult to satisfy, and that only under extreme conditions could an FRB be associated with an SGR burst.