Ubiquitous radio emission in quasars: Predominant AGN origin and a connection to jets, dust, and winds

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作者
Rivera, G. Calistro [1 ,2 ]
Alexander, D.M. [3 ]
Harrison, C.M. [4 ]
Fawcett, V.A. [4 ]
Best, P.N. [5 ]
Williams, W.L. [9 ]
Hardcastle, M.J. [6 ]
Rosario, D.J. [4 ]
Smith, D.J.B. [6 ]
Arnaudova, M.I. [6 ]
Escott, E. [3 ]
Gürkan, G. [6 ,10 ]
Kondapally, R. [4 ]
Miley, G. [7 ]
Morabito, L.K. [3 ,11 ]
Petley, J. [3 ]
Prandoni, I. [8 ]
Röttgering, H.J.A. [7 ]
Yue, B.-H. [5 ,7 ]
机构
[1] European Southern Observatory (ESO), Karl-Schwarzschild-Straße 2, Garching bei München,85748, Germany
[2] German Aerospace Center (DLR), Institute of Communications and Navigation, Wessling, Germany
[3] Centre for Extragalactic Astronomy, Department of Physics, Durham University, Durham,DH1 3LE, United Kingdom
[4] School of Mathematics, Statistics and Physics, Newcastle University, Newcastle upon Tyne,NE1 7RU, United Kingdom
[5] Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh,EH9 3HJ, United Kingdom
[6] Centre for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield,AL10 9AB, United Kingdom
[7] Leiden Observatory, Leiden University, PO Box 9513, Leiden,2300 RA, Netherlands
[8] INAF – Istituto di Radioastronomia, Via P. Gobetti 101, Bologna,40129, Italy
[9] SKA Observatory, Jodrell Bank, Lower Withington, Macclesfield,SK11 9FT, United Kingdom
[10] CSIRO Space and Astronomy, ATNF, PO Box 1130, Bentley,WA,6102, Australia
[11] Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham,DH1 3LE, United Kingdom
来源
Astronomy and Astrophysics | 1600年 / 691卷
基金
英国科学技术设施理事会; 英国科研创新办公室;
关键词
Active Galactic Nuclei - Adaptive optics - Aerodynamics - Black holes - Luminescence of liquids and solutions - Radio waves - White dwarfs;
D O I
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学科分类号
摘要
We present a comprehensive study of the physical origin of radio emission in optical quasars at redshifts z © The Authors 2024.
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