A candidate coherent radio flash following a neutron star merger

被引：1
|
作者：
Rowlinson, A. [1 ,2 ]
de Ruiter, I. [1 ]
Starling, R.L.C. [3 ]
Rajwade, K.M. [2 ]
Hennessy, A. [3 ]
Wijers, R.A.M.J. [1 ]
Anderson, G.E. [4 ]
Mevius, M. [2 ]
Ruhe, D. [1 ,5 ]
Gourdji, K. [6 ,7 ]
van der Horst, A.J. [8 ]
ter Veen, S. [2 ]
Wiersema, K. [9 ,10 ]
机构：
[1] Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, Amsterdam,NL-1098 XH, Netherlands
[2] ASTRON, Netherlands Institute for Radio Astronomy, Postbus 2, Dwingeloo,NL-7990 AA, Netherlands
[3] School of Physics and Astronomy, University of Leicester, University Road, Leicester,LE1 7RH, United Kingdom
[4] International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth,WA,6845, Australia
[5] AI4Science (AMLab), Informatics Institute, University of Amsterdam, Amsterdam,1098 XH, Netherlands
[6] Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn,VIC,3122, Australia
[7] ARC Centre of Excellence for Gravitational Wave Discovery, Hawthorn,VIC,3122, Australia
[8] Department of Physics, The George Washington University, 725 21st St NW, Washington,DC,20052, United States
[9] Physics Department, Lancaster University, Lancaster,LA1 4YB, United Kingdom
[10] Centre for Astrophysics Research, University of Hertfordshire, Hatfield,AL10 9AB, United Kingdom
来源：
Monthly Notices of the Royal Astronomical Society | 2024年 / 534卷 / 03期
关键词：
All Open Access; Gold;
D O I：
10.1093/mnras/stae2234
中图分类号：
学科分类号：
摘要：
Stars
引用
收藏
页码：2592 / 2608
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