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

被引：0

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：

暂无

中图分类号：

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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