机构

• 国家天文台 [2]
• 高能物理研究所 [1]
• 新疆天文台 [1]
• 云南天文台 [1]
• 国家授时中心 [1]

采集方式

• OAI收割 [6]

内容类型

• 期刊论文 [6]

发表日期

• 2020 [6]

学科主题

• 天文学 [1]
• 天文学::射电天文学 [1]

筛选

浏览/检索结果: 共6条，第1-6条 帮助 限定条件 发表日期：2020     条数/页： 5101520253035404550556065707580859095100 排序方式： 请选择提交时间升序提交时间降序发表日期升序发表日期降序题名升序题名降序作者升序作者降序 Repeating Fast Radio Bursts from Pulsar–Asteroid Belt Collisions: Frequency Drifting and Polarization 期刊论文  OAI收割 The Astrophysical Journal, 2020, 卷号: 905, 期号: 2 作者:  Liu,Ze-Nan;  Wang,Wei-Yang;  Yang,Yuan-Pei;  Dai,Zi-Gao   |  收藏  |  浏览/下载：14/0  |  提交时间：2021/12/06 Radio bursts  Asteroids  Minor planets  Neutron stars  Radio transient sources   Diverse polarization angle swings from a repeating fast radio burst source 期刊论文  OAI收割 NATURE, 2020, 卷号: 586, 期号: 7831, 页码: 693-+ 作者:  Luo, R.;  Wang, B. J.;  Men, Y. P.;  Zhang, C. F.;  Jiang, J. C.   |  收藏  |  浏览/下载：16/0  |  提交时间：2021/04/01 Diverse polarization angle swings from a repeating fast radio burst source 期刊论文  OAI收割 NATURE, 2020, 卷号: 586, 期号: 7831, 页码: 693-+ 作者:  Luo, R.;  Wang, B. J.;  Men, Y. P.;  Zhang, C. F.;  Jiang, J. C.   |  收藏  |  浏览/下载：19/0  |  提交时间：2021/03/29 Diverse polarization angle swings from a repeating fast radio burst source 期刊论文  OAI收割 NATURE, 2020, 卷号: 586, 期号: 7831, 页码: 693-+ 作者:  Luo, R.;  Wang, B. J.;  Men, Y. P.;  Zhang, C. F.;  Jiang, J. C.   |  收藏  |  浏览/下载：19/0  |  提交时间：2021/11/29 The Nearby Luminous Transient AT2018cow: A Magnetar Formed in a Subrelativistically Expanding Nonjetted Explosion 期刊论文  OAI收割 ASTROPHYSICAL JOURNAL LETTERS, 2020, 卷号: 888, 期号: 2, 页码: 9 作者:  Mohan, P.;  An, T.;  Yang, J.   |  收藏  |  浏览/下载：5/0  |  提交时间：2021/12/06 Transient sources  High energy astrophysics  Very long baseline interferometry  Magnetars  Burst astrophysics   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：37/0  |  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.